跳转到内容

恆星光度列表：修订间差异

维基百科，自由的百科全书
以互动方式浏览历史
←上一版本
删除的内容 添加的内容
可视化wikitext
小无编辑摘要
InternetArchiveBot（留言 | 贡献）
机器人
2,016,361次编辑
补救1个来源，并将0个来源标记为失效。) #IABot (v2.0.9.2
 
（未显示17个用户的29个中间版本）
第1行： 第1行：
下面的恆星列表是依據恆星的絕對熱星等增加（發光度減弱）的順序排列。[[絕對星等]]是恆星在距離地球10[[秒差距]]所呈現的[[視星等]]。絕對熱星等是測量恆星的發光度–一顆[[恆星]]每秒鐘所[[太陽輻射|輻射]]的總能量。這個表并不十分完整，因為一顆恆星的距離如果遠到我們看不到它，我們就無從得知它的發光度。一些參考資料所給的恆星發光度''非常''的不一樣（不同的順序或不同的恆星），這些恆星的不同數據資料有些不見得是不可靠，而是注意的和分析時注重的物理資訊不同和有實際上的困難。
{{copyedit|time=2010-08-15T03:32:48+00:00}}
下面的恆星列表是依據恆星的絕對[[熱星等]]增加（[[發光度]]減弱）的順序排列。絕對星等是恆星在距離地球10[[秒差距]]所呈現的[[視星等]]。絕對熱星等是測量恆星的發光度–一顆[[恆星]]每秒鐘所[[太陽輻射|輻射]]的總能量。


{{Expand list|date=2021年7月}}<!-- 請不要移除此標記，直到全宇宙地圖繪製完成 -->
這個表不是很完整的，因為一顆恆星的距離如果遠到我們看不到它，我們就無從得知它的發光度。一些參考資料所給的恆星發光度''非常''的不一樣（不同的順序或不同的恆星），這些恆星的不同數據資料有些不見得是不可靠，而是注意的和分析時注重的物理資訊不同和有實際上的困難。將它們不同的資料（參見[[手槍星]]的例子）成套的收錄在表中只是為了比較（它們有些不在已知最亮的恆星之中）。


{| class="wikitable floatright" style="width: 150px;"
|+'''图例'''
| style="background: {{star-color|WC}};" align="center" |[[沃尔夫-拉叶星]]
|-
| style="background: {{star-color|WN}};" align="center" |[[高光度蓝变星]]
|-
| style="background: {{star-color|O}};" align="center" |[[O型星]]
|-
| style="background: {{star-color|B}};" align="center" |[[恒星光谱#B型|B型星]]
|-
|}
'''太陽光度1百萬倍以上的恒星：'''
{| class="wikitable sortable"
{| class="wikitable sortable"
!恒星名称
![[輻射熱光度]](太陽=1)
![[絕對熱星等]]
!距離([[光年]])
![[视星等]]
![[有效温度]]([[开尔文|K]])
!链接
!參考文獻
|-
|-
! style="background:#efefef;" | 恆星名字
| style="background: {{star-color|WC}};" |[[R136a1]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|6166000
! 視星等
| -12.235
! style="background:#ffdead;" | 絕對星等
|163000
! style="background:#afdead;" | 太陽光度（太陽=1）
|12.28
|46000
|{{SIMBAD link|RMC136a1|SIMBAD}}
|<ref name="bestenlehner2020">{{cite journal|last1=Bestenlehner|first1=Joachim M.|last2=Crowther|first2=Paul A.|last3=Caballero-Nieves|first3=Saida M.|last4=Schneider|first4=Fabian R. N.|last5=Simón-Díaz|first5=Sergio|last6=Brands|first6=Sarah A.|last7=De Koter|first7=Alex|last8=Gräfener|first8=Götz|last9=Herrero|first9=Artemio|last10=Langer|first10=Norbert|last11=Lennon|first11=Daniel J.|year=2020|title=The R136 star cluster dissected with Hubble Space Telescope/STIS. II. Physical properties of the most massive stars in R136|journal=Monthly Notices of the Royal Astronomical Society|volume=499|issue=2|page=1918|arxiv=2009.05136|bibcode=2020MNRAS.499.1918B|doi=10.1093/mnras/staa2801|first14=Jorick S.|last14=Vink|first13=Joachim|last13=Puls|first12=Jesus|last12=Maíz Apellániz|s2cid=221640940}}</ref><ref name="Doran2013">{{Cite journal|last1=Doran|first1=E. I.|last2=Crowther|first2=P. A.|last3=de Koter|first3=A.|last4=Evans|first4=C. J.|last5=McEvoy|first5=C.|last6=Walborn|first6=N. R.|last7=Bastian|first7=N.|last8=Bestenlehner|first8=J. M.|last9=Gräfener|first9=G.|last10=Herrero|first10=A.|last11=Köhler|first11=K.|date=2013|title=The VLT-FLAMES Tarantula Survey. XI. A census of the hot luminous stars and their feedback in 30 Doradus|journal=Astronomy & Astrophysics|volume=558|issue=134|page=30|arxiv=1308.3412|bibcode=2013A&A...558A.134D|doi=10.1051/0004-6361/201321824|first13=F.|first17=W. D.|last17=Taylor|last12=Maíz Apellániz|last13=Najarro|last14=Puls|first18=J. Th.|first12=J.|first16=F. R. N.|first19=J. S.|first14=J.|last15=Sana|last16=Schneider|last18=van Loon|last19=Vink|first15=H.|s2cid=118510909}}</ref>
|-
|-
| [[R136a1]]（在[[大麥哲倫星系]]）
| style="background: {{star-color|WC}};" |[[R136a2]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|5623000
|
| −12.9
| -12.135
|163000
| 8,500,000
|12.34
|50000
|{{SIMBAD link|RMC136a2|SIMBAD}}
|<ref name="bestenlehner2020" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[BAT99-98]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[天鵝座OB2-12|天鵝座OB2#12]]
|5012000
|  
| −12.2
| -12.01
|165000
| 6,000,000
|13.38
|45000
|{{SIMBAD link|BAT99+98|SIMBAD}}
|<ref name="hainich">{{Cite journal|last1=Hainich|first1=R.|last2=Rühling|first2=U.|last3=Todt|first3=H.|last4=Oskinova|first4=L. M.|last5=Liermann|first5=A.|last6=Gräfener|first6=G.|last7=Foellmi|first7=C.|last8=Schnurr|first8=O.|last9=Hamann|first9=W. -R.|year=2014|title=The Wolf-Rayet stars in the Large Magellanic Cloud|journal=Astronomy & Astrophysics|volume=565|page=A27|arxiv=1401.5474|bibcode=2014A&A...565A..27H|doi=10.1051/0004-6361/201322696|s2cid=55123954}}</ref><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WN}};" |[[G0.238-0.071]] (位于[[银心]])
| [[HD 93129A]]
|5012000
| 6.97
| −12.1
| -12.01
|26000
| 5,500,000
|14.37 (J波段)
|39500-44000
|{{SIMBAD link|MCD2010+G0.238-0.071|SIMBAD}}
|<ref name="mcd2010">{{Cite journal|last1=Mauerhan|first1=J. C.|last2=Cotera|first2=A.|last3=Dong|first3=H.|last4=Morris|first4=M. R.|last5=Wang|first5=Q. D.|last6=Stolovy|first6=S. R.|last7=Lang|first7=C.|year=2010|title=Isolated Wolf-Rayet Stars and O Supergiants in the Galactic Center Region Identified Via Paschen-α Excess|journal=The Astrophysical Journal|volume=725|issue=1|pages=188–199|arxiv=1009.2769|bibcode=2010ApJ...725..188M|doi=10.1088/0004-637X/725/1/188|s2cid=20968628}}</ref><ref name="HBSP">{{Cite journal|last1=Dong|first1=H.|last2=Wang|first2=Q. D.|last3=Cotera|first3=A.|last4=Stolovy|first4=S.|last5=Morris|first5=M. R.|last6=Mauerhan|first6=J.|last7=Mills|first7=E. A.|last8=Schneider|first8=G.|last9=Calzetti|first9=D.|last10=Lang|first10=C.|date=2011-10-11|title=Hubble Space Telescope Paschen α survey of the Galactic Centre: data reduction and products: HST/NICMOS Paschen α survey of the GC|url=https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2011.19013.x|journal=Monthly Notices of the Royal Astronomical Society|volume=417|issue=1|pages=114–135|arxiv=1105.1703|bibcode=2011MNRAS.417..114D|doi=10.1111/j.1365-2966.2011.19013.x|s2cid=11060463|access-date=2021-07-11|archive-date=2017-07-07|archive-url=https://web.archive.org/web/20170707063556/https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2011.19013.x|dead-url=no}}</ref>
|-
|-
| style="background: {{star-color|O}};" |[[M33-013406.63]] A (位于[[三角座星系]])
| [[海山二]]
|4677000
| 3.9 到 10.5
| −12.1
| -11.935
|3000000
| 5,500,000
|16.084
|30000
|{{SIMBAD link|LGGS+J013406.63%2B304147.8|SIMBAD}}
|<ref name=":2">{{Cite journal|last1=Kourniotis|first1=M|last2=Kraus|first2=M|last3=Arias|first3=M L|last4=Cidale|first4=L|last5=Torres|first5=A F|date=2018-11-01|title=On the evolutionary state of massive stars in transition phases in M33|url=https://academic.oup.com/mnras/article/480/3/3706/5063594|journal=Monthly Notices of the Royal Astronomical Society|volume=480|issue=3|pages=3706–3717|arxiv=1808.00008|bibcode=2018MNRAS.480.3706K|doi=10.1093/mnras/sty2087|issn=0035-8711|access-date=2021-07-11|archive-date=2022-02-14|archive-url=https://web.archive.org/web/20220214144743/https://academic.oup.com/mnras/article/480/3/3706/5063594|dead-url=no}}</ref><ref name=":4">{{Cite journal|last1=Massey|first1=Philip|last2=Olsen|first2=K. A. G.|last3=Hodge|first3=Paul W.|last4=Strong|first4=Shay B.|last5=Jacoby|first5=George H.|last6=Schlingman|first6=Wayne|last7=Smith|first7=R. C.|date=2006|title=A Survey of Local Group Galaxies Currently Forming Stars. I. UBVRI Photometry of Stars in M31 and M33|url=https://iopscience.iop.org/article/10.1086/503256|journal=The Astronomical Journal|volume=131|issue=5|pages=2478–2496|arxiv=astro-ph/0602128|bibcode=2006AJ....131.2478M|doi=10.1086/503256|issn=0004-6256|s2cid=118865956|access-date=2021-07-11|archive-date=2020-06-10|archive-url=https://web.archive.org/web/20200610105838/https://iopscience.iop.org/article/10.1086/503256|dead-url=no}}</ref>
|-
|-
| style="background: {{star-color|WN}};" |[[海山二]] A (位于[[船底座星云]]内的[[川普勒16]])
| [[LBV 1806-20]]
|4600000
| 8.6
| −12.0
| -11.917
|7500
| 5,000,000 [http://arxiv.org/abs/astro-ph/0404435]
| style="background: lightblue;" |4.3
|9400-35200
|{{SIMBAD link|Eta+Carinae|SIMBAD}}
|<ref name="mehner2019">{{cite journal|last1=Mehner|first1=A.|last2=De Wit|first2=W.-J.|last3=Asmus|first3=D.|last4=Morris|first4=P. W.|last5=Agliozzo|first5=C.|last6=Barlow|first6=M. J.|last7=Gull|first7=T. R.|last8=Hillier|first8=D. J.|last9=Weigelt|first9=G.|year=2019|title=Mid-infrared evolution of η Carinae from 1968 to 2018|journal=Astronomy & Astrophysics|volume=630|page=L6|arxiv=1908.09154|bibcode=2019A&A...630L...6M|doi=10.1051/0004-6361/201936277|s2cid=202149820}}</ref><ref name="2018-07-02_NAL">{{cite journal|last1=Hamaguchi|first1=Kenji|last2=Corcoran|first2=Michael F|last3=Pittard|first3=Julian M|last4=Sharma|first4=Neetika|last5=Takahashi|first5=Hiromitsu|last6=Russell|first6=Christopher M. P|last7=Grefenstette|first7=Brian W|last8=Wik|first8=Daniel R|last9=Gull|first9=Theodore R|last10=Richardson|first10=Noel D|last11=Madura|first11=Thomas I|year=2018|title=Non-thermal X-rays from colliding wind shock acceleration in the massive binary Eta Carinae|url=https://doi.org/10.1038/s41550-018-0505-1|journal=Nature Astronomy|volume=2|issue=9|pages=731–736|arxiv=1904.09219|bibcode=2018NatAs.tmp...87H|doi=10.1038/s41550-018-0505-1|archive-url=https://web.archive.org/web/20200223030219/https://www.nature.com/articles/s41550-018-0505-1?error=cookies_not_supported&code=72e043e7-127c-40b9-9ffb-95fbff9faa1a|archive-date=2020-02-23|s2cid=126188024|first12=Anthony F. J|last12=Moffat|access-date=2021-07-11|dead-url=no}}</ref>
|-
|-
| style="background: {{star-color|WC}};" |[[R136a3]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[QPM-241]]
|4266000
|  
| −11.9
| -11.835
|163000
| 4,500,000
|12.97
|50000
|{{SIMBAD link|RMC136a3|SIMBAD}}
|<ref name="bestenlehner2020" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|O}};" |[[Sk -69° 249]] A (位于[[大麦哲伦星系]]内的[[NGC 2074]])
| [[HDE 319718]]
|4130000
|  
| −11.8
| -11.8
|160000
| 4,200,000
|10.68
|38900
|{{SIMBAD link|Sk+-69+249|SIMBAD}}
|<ref name=":42">{{Cite journal|last1=Massey|first1=Philip|last2=Waterhouse|first2=Elizabeth|last3=DeGioia-Eastwood|first3=Kathleen|date=May 2000|title=The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster Turnoffs. I. Results from 19 OB Associations in the Magellanic Clouds|url=https://iopscience.iop.org/article/10.1086/301345|journal=The Astronomical Journal|volume=119|issue=5|pages=2214–2241|arxiv=astro-ph/0002233|bibcode=2000AJ....119.2214M|doi=10.1086/301345|s2cid=16891188|access-date=2021-07-11|archive-date=2020-10-30|archive-url=https://web.archive.org/web/20201030140505/https://iopscience.iop.org/article/10.1086/301345|dead-url=no}}</ref><ref name="zacharias" />
|-
|-
| style="background: {{star-color|WN}};" |[[人马座V4998]] (靠近[[五合星团]])
| [[WR 102ka]]
|3981000
|  
| −11.6
| -11.76
|25000
| 3,700,000
|12.534 (J波段)
|12000
|{{SIMBAD link|V4998+Sagittarii|SIMBAD}}
|<ref name="mauerhan">{{Cite journal|last1=Mauerhan|first1=J. C.|last2=Morris|first2=M. R.|last3=Cotera|first3=A.|last4=Dong|first4=H.|last5=Wang|first5=Q. D.|last6=Stolovy|first6=S. R.|last7=Lang|first7=C.|last8=Glass|first8=I. S.|year=2010|title=Discovery of a Luminous Blue Variable with an Ejection Nebula Near the Quintuplet Cluster|journal=The Astrophysical Journal|volume=713|issue=1|pages=L33–L36|arxiv=1002.3379|bibcode=2010ApJ...713L..33M|doi=10.1088/2041-8205/713/1/L33|s2cid=42696538}}</ref><ref name=":3">{{Cite journal|last1=Cutri|first1=R. M.|last2=Skrutskie|first2=M. F.|last3=Van Dyk|first3=S.|last4=Beichman|first4=C. A.|last5=Carpenter|first5=J. M.|last6=Chester|first6=T.|last7=Cambresy|first7=L.|last8=Evans|first8=T.|last9=Fowler|first9=J.|last10=Gizis|first10=J.|last11=Howard|first11=E.|date=2003|title=VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)|journal=VizieR On-line Data Catalog|bibcode=2003yCat.2246....0C|last22=Weinberg|last20=Stiening|first20=R.|last21=Sykes|first21=M.|last24=Wheelock|first22=M.|last23=Wheaton|first23=W. A.|first24=S.|first12=J.|last19=Schneider|first19=S.|first17=K. A.|last25=Zacarias|last18=McCallon|last12=Huchra|first18=H.|last13=Jarrett|last14=Kopan|first14=E. L.|last15=Kirkpatrick|first13=T.|last16=Light|first16=R. M.|last17=Marsh|first15=J. D.|first25=N.}}</ref>
|-
|-
| [[HD 5980]]（在[[小麦哲伦星系]]）
| style="background: {{star-color|WC}};" |[[R136c]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|3802000
|  
| −11.5
| -11.71
|163000
| 3,300,000
|13.43
|-
|51000
| [[VFTS 682]]（在[[大麥哲倫星系]]）
|{{SIMBAD link|RMC136c|SIMBAD}}
|
|<ref name="schneider2018">{{cite journal|last1=Schneider|first1=F. R. N.|last2=Sana|first2=H.|last3=Evans|first3=C. J.|last4=Bestenlehner|first4=J. M.|last5=Castro|first5=N.|last6=Fossati|first6=L.|last7=Gräfener|first7=G.|last8=Langer|first8=N.|last9=Ramírez-Agudelo|first9=O. H.|last10=Sabín-Sanjulián|first10=C.|last11=Simón-Díaz|first11=S.|year=2018|title=An excess of massive stars in the local 30 Doradus starburst|journal=Science|volume=359|issue=6371|pages=69–71|arxiv=1801.03107|bibcode=2018Sci...359...69S|doi=10.1126/science.aan0106|pmid=29302009|last26=Najarro|first12=F.|last13=Crowther|first13=P. A.|last14=de Koter|first15=S. E.|last16=Dufton|last17=Garcia|first17=M.|first16=P. L.|last18=Gieles|last19=Hénault-Brunet|first19=V.|first18=M.|last20=Herrero|first20=A.|last21=Izzard|first32=C.|last12=Tramper|first21=R. G.|first25=N.|last22=Kalari|first22=V.|first14=A.|first23=D. J.|last24=Maíz Apellániz|first24=J.|last25=Markova|first26=F.|last27=Podsiadlowski|last28=Puls|first28=J.|last15=de Mink|last29=Taylor|last30=van Loon|first29=W. D.|first30=J. Th.|last31=Vink|first31=J. S.|last32=Norman|last23=Lennon|first27=Ph.|s2cid=206658504}}</ref><ref name="Doran2013" />
| -11.33
| 3,000,000
|-
|-
| [[HDE 269810]]（在[[大麥哲倫星系]]）
| style="background: {{star-color|O}};" |[[BAT99-105]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|3631000
|  
| −11.1
| -11.66
|163000
| 2,200,000[http://arxiv.org/abs/astro-ph/0403557]
|12.78
|47300
|{{SIMBAD link|Cl*+NGC+2070+MEL+42|SIMBAD}}
|<ref name="best">{{cite journal|last1=Bestenlehner|first1=J. M.|last2=Gräfener|first2=G.|last3=Vink|first3=J. S.|last4=Najarro|first4=F.|last5=De Koter|first5=A.|last6=Sana|first6=H.|last7=Evans|first7=C. J.|last8=Crowther|first8=P. A.|last9=Hénault-Brunet|first9=V.|last10=Herrero|first10=A.|last11=Langer|first11=N.|year=2014|title=The VLT-FLAMES Tarantula Survey. XVII. Physical and wind properties of massive stars at the top of the main sequence|journal=Astronomy & Astrophysics|volume=570|page=A38|arxiv=1407.1837|bibcode=2014A&A...570A..38B|doi=10.1051/0004-6361/201423643|last13=Simón-Díaz|first13=S.|last14=Taylor|first14=W. D.|last15=Walborn|first15=N. R.|first12=F. R. N.|last12=Schneider|s2cid=118606369}}</ref><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[默瑟23]]-2 (位于靠近[[银河平面]]的[[默瑟23]])
| [[Var 83]]（在[[三角座星系]]）
|3631000
|  
| −11.1
| -11.66
|21200
| 2,200,000[http://adsabs.harvard.edu/cgi-bin/bib_query?1996A%26A...314..131S]
|8.646 (J波段)
|38000
|{{SIMBAD link|HKB2010b+Obj2|SIMBAD}}
|<ref name=":20">{{Cite journal|last=Hanson|first=M. M.|last2=Kurtev|first2=R.|last3=Borissova|first3=J.|last4=Georgiev|first4=L.|last5=Ivanov|first5=V. D.|last6=Hillier|first6=D. J.|last7=Minniti|first7=D.|date=June 2010|title=Obscured clusters: III. Follow-up observations of Mercer 23|url=http://www.aanda.org/10.1051/0004-6361/200913122|journal=Astronomy and Astrophysics|volume=516|page=A35|bibcode=2010A&A...516A..35H|doi=10.1051/0004-6361/200913122|issn=0004-6361|doi-access=free|s2cid=53705451}}</ref><ref name=":3" />
|-
|-
| style="background: {{star-color|O}};" |[[G0.070+0.025]] (位于[[银心]])
| [[Wray 17-96]]
|3311000
|  
| −10.9
| -11.56
|26000
| 1,800,000[http://www.journals.uchicago.edu/ApJ/journal/issues/ApJ/v572n1/52967/52967.web.pdf]
|14.799 (J波段)
|45000
|{{SIMBAD link|MCD2010+G0.070%2B0.025|SIMBAD}}
|<ref name="mcd2010" />
|-
|-
| style="background: {{star-color|WN}};" |[[手枪星]] (位于[[五合星团]])
| [[手槍星]]
|3300000
|  
| −10.8
| -11.556
|25000
| 1,700,000
|11.79 (J波段)
|11800
|{{SIMBAD link|Pistol+Star|SIMBAD}}
|<ref name="ryan">{{cite journal|last1=Lau|first1=R. M.|last2=Herter|first2=T. L.|last3=Morris|first3=M. R.|last4=Adams|first4=J. D.|year=2014|title=Nature Versus Nurture: Luminous Blue Variable Nebulae in and Near Massive Stellar Clusters at the Galactic Center|journal=The Astrophysical Journal|volume=785|issue=2|page=120|arxiv=1403.5298|bibcode=2014ApJ...785..120L|doi=10.1088/0004-637X/785/2/120|s2cid=118447462}}</ref><ref name="qc">{{Cite journal|last1=Clark|first1=J. S.|last2=Lohr|first2=M. E.|last3=Patrick|first3=L. R.|last4=Najarro|first4=F.|last5=Dong|first5=H.|last6=Figer|first6=D. F.|date=2018|title=An updated stellar census of the Quintuplet cluster|url=https://www.aanda.org/10.1051/0004-6361/201833041|journal=Astronomy & Astrophysics|volume=618|page=A2|arxiv=1805.10139|bibcode=2018A&A...618A...2C|doi=10.1051/0004-6361/201833041|issn=0004-6361|s2cid=53501337}}</ref>
|-
|-
| style="background: {{star-color|WC}};" |[[默瑟30]]-1 A (位于[[龙鱼星云]]内的[[默瑟30]])
| [[仙女座AF]]（在[[仙女座星系]]）
|3236000
|  
| −10.8
| -11.535
|40000
| 1,600,000[http://adsabs.harvard.edu/cgi-bin/bib_query?1996A%26A...314..131S]
|10.33 (J波段)
|32200
|{{SIMBAD link|DNB2016+Mc30-1|SIMBAD}}
|<ref name=":17">{{Cite journal|last=de la Fuente|first=D.|last2=Najarro|first2=F.|last3=Borissova|first3=J.|last4=Ramírez Alegría|first4=S.|last5=Hanson|first5=M. M.|last6=Trombley|first6=C.|last7=Figer|first7=D. F.|last8=Davies|first8=B.|last9=Garcia|first9=M.|last10=Kurtev|first10=R.|last11=Urbaneja|first11=M. A.|date=May 2016|title=Probing the Dragonfish star-forming complex: the ionizing population of the young massive cluster Mercer 30|url=http://www.aanda.org/10.1051/0004-6361/201528004|journal=Astronomy & Astrophysics|volume=589|page=A69|arxiv=1602.02503|bibcode=2016A&A...589A..69D|doi=10.1051/0004-6361/201528004|issn=0004-6361|last12=Smith|first12=L. C.|last13=Lucas|first13=P. W.|last14=Herrero|first14=A.|s2cid=119096455}}</ref>
|-
|-
| style="background: {{star-color|WC}};" |[[VFTS 682]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[Var B]]（在[[三角座星系]]）
|3236000
|  
| −10.4
| -11.535
|164000
| 1,100,000[http://adsabs.harvard.edu/cgi-bin/bib_query?1996A%26A...314..131S]
|16.08
|52200
|{{SIMBAD link|VFTS+682|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[WR 42e]] (位于[[NGC 3603]]内的[[HD 97950]])
| [[船底座AG]]
|3200000
| 7.1 到 9.0
| −10.3
| -11.523
|25000
| 1,000,000[http://arxiv.org/abs/astro-ph/0512372]
|14.53
|43000
|{{SIMBAD link|WR+42e|SIMBAD}}
|<ref name="lopes">{{Cite journal|last1=Roman-Lopes|first1=A.|year=2012|title=A Galactic O2 If*/WN6 star possibly ejected from its birthplace in NGC 3603|journal=Monthly Notices of the Royal Astronomical Society Letters|volume=427|issue=1|pages=L65–L69|arxiv=1209.1598|bibcode=2012MNRAS.427L..65R|doi=10.1111/j.1745-3933.2012.01346.x|s2cid=118453639}}</ref>
|-
|-
| style="background: {{star-color|WC}};" |[[牡丹星]] (靠近[[银心]])
| [[劍魚座S]]
|3162000
| 8.6 到 11.8
| −10.1
| -11.51
|26000
| 870,000
|12.978 (J波段)
|25100
|{{SIMBAD link|Peony+Star|SIMBAD}}
|<ref name="barniske">{{Cite journal|last1=Barniske|first1=A.|last2=Oskinova|first2=L. M.|last3=Hamann|first3=W. -R.|year=2008|title=Two extremely luminous WN stars in the Galactic center with circumstellar emission from dust and gas|journal=Astronomy and Astrophysics|volume=486|issue=3|page=971|arxiv=0807.2476|bibcode=2008A&A...486..971B|doi=10.1051/0004-6361:200809568|s2cid=8074261}}</ref><ref name=":3" />
|-
|-
| style="background: {{star-color|WN}};" |[[R99]] (位于[[大麦哲伦星系]]内的[[N44]])
| [[弧矢增二十二]]
|3162000
| 2.21
| −10
| -11.51
|163000
| 790,000
|11.52
|28000
|{{SIMBAD link|RMC99|SIMBAD}}
|<ref name="hainich" /><ref name="ducati">{{cite journal|last1=Ducati|first1=J. R.|year=2002|title=VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system|journal=CDS/ADC Collection of Electronic Catalogues|volume=2237|page=0|bibcode=2002yCat.2237....0D}}</ref>
|-
|-
| [[Var C]]（在[[三角座星系]]）
| style="background: {{star-color|WN}};" |[[Var A-1]] (位于[[仙女座星系]])
|3133000
|  
| −9.8
| -11.5
|2500000
| 660,000[http://adsabs.harvard.edu/cgi-bin/bib_query?1996A%26A...314..131S]
|17.143
|20400-28100
|{{SIMBAD link|RB73+A-1|SIMBAD}}
|<ref name="m31">{{Cite journal|last1=Sholukhova|first1=O.|last2=Bizyaev|first2=D.|last3=Fabrika|first3=S.|last4=Sarkisyan|first4=A.|last5=Malanushenko|first5=V.|last6=Valeev|first6=A.|date=2014|title=New Luminous Blue Variables in the Andromeda galaxy|journal=Monthly Notices of the Royal Astronomical Society|volume=447|issue=3|pages=2459–2467|arxiv=1412.5319|bibcode=2015MNRAS.447.2459S|doi=10.1093/mnras/stu2597|s2cid=118374186}}</ref><ref name=":4" />
|-
|-
| style="background: {{star-color|WC}};" |[[VFTS 1022]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[仙后座ρ]]
|3020000
| 4.4
| −9.6
| -11.46
|164000
| 550,000
|13.47
|42200
|{{SIMBAD link|VFTS+1022|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[WR 24]] (位于[[船底座星云]]的[[科林德目录|科林德228]])
| [[船底座HR]]
|2951000
|  
| −9.5
| -11.435
|8200
| 500,000[http://www.edpsciences.org/articles/aa/pdf/2002/19/aa2089.pdf]
| style="background: lightblue;" |6.48
|50100
|{{SIMBAD link|WR+24|SIMBAD}}
|<ref name="WN">{{cite journal|last1=Sota|first1=A.|last2=Maíz Apellániz|first2=J.|last3=Morrell|first3=N. I.|last4=Barbá|first4=R. H.|last5=Walborn|first5=N. R.|last6=Gamen|first6=R. C.|last7=Arias|first7=J. I.|last8=Alfaro|first8=E. J.|last9=Oskinova|first9=L. M.|year=2019|title=The Galactic WN stars revisited. Impact of Gaia distances on fundamental stellar parameters|journal=Astronomy & Astrophysics|volume=A57|page=625|arxiv=1904.04687|bibcode=2019A&A...625A..57H|doi=10.1051/0004-6361/201834850|s2cid=104292503}}</ref><ref name="gcvs">{{cite journal|last1=Samus|first1=N. N.|last2=Durlevich|first2=O. V.|display-authors=etal|year=2009|title=VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)|journal=VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S|volume=1|bibcode=2009yCat....102025S}}</ref>
|-
|-
| style="background: {{star-color|WC}};" |[[CXOGC J174528.6-285605]] (位于[[银心]])
| [[仙女座AE]]（在[[仙女座星系]]）
|2884000
|  
| −9.4
| -11.41
|26000
| 450,000[http://adsabs.harvard.edu/cgi-bin/bib_query?1996A%26A...314..131S]
|14.46 (J波段)
|30000
|{{SIMBAD link|CXOGC+J174528.6-285605|SIMBAD}}
|<ref name=":21">{{Cite journal|last=Mauerhan|first=J. C.|last2=Muno|first2=M. P.|last3=Morris|first3=M. R.|last4=Stolovy|first4=S. R.|last5=Cotera|first5=A.|date=10 February 2010|title=Near-infrared Counterparts to Chandra X-ray Sources Toward the Galactic Center. II. Discovery of Wolf-Rayet Stars and O Supergiants|url=https://iopscience.iop.org/article/10.1088/0004-637X/710/1/706|journal=The Astrophysical Journal|volume=710|issue=1|pages=706–728|arxiv=0912.1055|bibcode=2010ApJ...710..706M|doi=10.1088/0004-637X/710/1/706|issn=0004-637X|s2cid=32339182|access-date=2021-07-11|archive-date=2021-04-10|archive-url=https://web.archive.org/web/20210410161242/https://iopscience.iop.org/article/10.1088/0004-637X/710/1/706|dead-url=no}}</ref>
|-
|-
| style="background: {{star-color|WN}};" |[[G0.059-0.068]] (位于[[银心]])
| [[大犬座VY]]
|2884000
| 7.95
| −9.4
| -11.41
|26000
| 450,000[http://arxiv.org/pdf/astro-ph/0610433]
|13.337 (J波段)
|39500-44000
|{{SIMBAD link|MCD2010+G0.059-0.068|SIMBAD}}
|<ref name="mcd2010" /><ref name="HBSP" />
|-
|-
| style="background: {{star-color|WC}};" |[[NGC 3603-B|HD 97950 B]] (位于[[NGC 3603]]内的[[HD 97950]])
| [[司怪三]]
|2884000
| 4.65
| −9.3
| -11.41
|24000
| 420,000
|11.33
|42000
|{{SIMBAD link|HD+97950B|SIMBAD}}
|<ref name="crowther">{{Cite journal|last1=Crowther|first1=P. A.|last2=Schnurr|first2=O.|last3=Hirschi|first3=R.|last4=Yusof|first4=N.|last5=Parker|first5=R. J.|last6=Goodwin|first6=S. P.|last7=Kassim|first7=H. A.|year=2010|title=The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M<sub>⊙</sub> stellar mass limit|journal=[[Monthly Notices of the Royal Astronomical Society]]|volume=408|issue=2|pages=731–751|arxiv=1007.3284|bibcode=2010MNRAS.408..731C|doi=10.1111/j.1365-2966.2010.17167.x|s2cid=53001712}}</ref><ref name="melena2008">{{cite journal|last1=Melena|first1=Nicholas W.|last2=Massey|first2=Philip|last3=Morrell|first3=Nidia I.|last4=Zangari|first4=Amanda M.|year=2008|title=The Massive Star Content of NGC 3603|url=https://archive.org/details/sim_astronomical-journal_2008-03_135_3/page/878|journal=The Astronomical Journal|volume=135|issue=3|pages=878–891|arxiv=0712.2621|bibcode=2008AJ....135..878M|doi=10.1088/0004-6256/135/3/878|issn=0004-6256|s2cid=16765414}}</ref>
|-
|-
| style="background: {{star-color|WC}};" |[[BAT99-116]] A (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[HDE 226868]]
|2692000
| 8.9
| −9.25
| -11.335
|163000
| 390,000
|13.09
|53000
|{{SIMBAD link|Cl*+NGC+2070+MEL+34|SIMBAD}}
|<ref name="tehrani">{{cite journal|last1=Tehrani|first1=Katie A.|last2=Crowther|first2=Paul A.|last3=Bestenlehner|first3=Joachim M.|last4=Littlefair|first4=Stuart P.|last5=Pollock|first5=A M T.|last6=Parker|first6=Richard J.|last7=Schnurr|first7=Olivier|year=2019|title=Weighing Melnick 34: The most massive binary system known|journal=Monthly Notices of the Royal Astronomical Society|volume=484|issue=2|pages=2692–2710|arxiv=1901.04769|bibcode=2019MNRAS.484.2692T|doi=10.1093/mnras/stz147|s2cid=119069481}}</ref><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[WR 102hb]] (位于[[五合星团]])
| [[參宿二]]
|2630000
| 1.70
| −9.2
| -11.31
|26000
| 380,000
|13.9 (J波段)
|25100
|{{SIMBAD link|WR+102hb|SIMBAD}}
|<ref name="quintuplet">{{Cite journal|last1=Liermann|first1=A.|last2=Hamann|first2=W. -R.|last3=Oskinova|first3=L. M.|last4=Todt|first4=H.|last5=Butler|first5=K.|year=2010|title=The Quintuplet cluster|journal=Astronomy & Astrophysics|volume=524|page=A82|arxiv=1011.5796|bibcode=2010A&A...524A..82L|doi=10.1051/0004-6361/200912612|s2cid=30091594}}</ref><ref name="qc" />
|-
|-
| style="background: {{star-color|WC}};" |[[BAT99-80]] A (位于[[大麦哲伦星系]]内的[[NGC 2044]])
| [[人馬座KW]]
|2512000
|  
| −9.17
| -11.26
|165000
| 370,000
|13
|45000
|{{SIMBAD link|BAT99+80|SIMBAD}}
|<ref name="hainich" /><ref name="Schild">{{Cite journal|last1=Schild|first1=H.|last2=Testor|first2=G.|date=March 1992|title=Spectral types and UBV magnitudes of stars in the 30 Doradus complex.|url=https://ui.adsabs.harvard.edu/abs/1992A%26AS...92..729S/abstract|journal=Astronomy and Astrophysics Supplement Series|volume=92|pages=729–748|bibcode=1992A&AS...92..729S|s2cid=115371295}}</ref>
|-
|-
| style="background: {{star-color|WC}};" |[[R146]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[仙王座V354]]
|2512000
|  
| −9.15
| -11.26
|164000
| 360,000
|13.11
|63000
|{{SIMBAD link|RMC146|SIMBAD}}
|<ref name="hainich" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[VFTS 482]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[仙王座μ]]
|2512000
| 4.04
| −9.08
| -11.26
|164000
| 340,000
|12.95
|42200
|{{SIMBAD link|VFTS+482|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[NGC 3603-A1|HD 97950 A1a]] (位于[[NGC 3603]]内的[[HD 97950]])
| [[仙王座VV|仙王座VV A]]
|2455000
|  
| −9.0
| -11.235
|24000
| 315,000
|11.18
|42000
|{{SIMBAD link|Cl*+NGC+3603+BLW+A1|SIMBAD}}
|<ref name="crowther" /><ref name="melena2008" />
|-
|-
| style="background: {{star-color|WC}};" |[[WR 102ea]] (位于[[五合星团]])
| [[WOH G64]]
|2455000
|  
| −
| -11.235
|26000
| 280,000
|13.18 (J波段)
|25100
|{{SIMBAD link|WR+102ea|SIMBAD}}
|<ref name="quintuplet" /><ref name="qc" />
|-
|-
| style="background: {{star-color|WC}};" |[[CXOGC J174516.1-284909]] (位于[[银心]])
| [[天鵝座KY]]
|2399000
|  
| −8.84
| -11.21
|26000
| 270,000
|11.49 (J波段)
|20000
|{{SIMBAD link|CXOGC+J174516.1-284909|SIMBAD}}
|<ref name=":21" />
|-
|-
| style="background: {{star-color|WC}};" |[[CXOGC J174711.4-283006]] (位于[[银心]])
| [[天津四]]
|2399000
| 1.25
| −8.73
| -11.21
|26000
| 250,000
|16.56 (J波段)
|30000
|{{SIMBAD link|CXOGC+J174711.4-283006|SIMBAD}}
|<ref name=":21" />
|-
|-
| style="background: {{star-color|WC}};" |[[WR 25]] A (位于[[船底座星云]]内的[[川普勒16]])
| [[Theta1 Orionis C]]
|2399000
| 5.13
| −8.6
| -11.21
|6800
| 220,000
|8.8
|50100
|{{SIMBAD link|WR+25|SIMBAD}}
|<ref name="WN" /><ref name="ducati" />
|-
|-
| style="background: {{star-color|WN}};" |[[LGGS J004444.52+412804.0]] (位于[[仙女座星系]])
| [[参宿一]]
|2377000
| 1.79
| −7.8
| -11.2
|2500000
| 100,000
|18.1
|7000-18000
|{{SIMBAD link|LGGS+J004444.52%2B412804.0|SIMBAD}}
|<ref name="m31" /><ref>{{Cite journal|last1=Humphreys|first1=Roberta M.|last2=Weis|first2=Kerstin|last3=Davidson|first3=Kris|last4=Bomans|first4=D. J.|last5=Burggraf|first5=Birgitta|date=2014-07-02|title=LUMINOUS AND VARIABLE STARS IN M31 AND M33. II. LUMINOUS BLUE VARIABLES, CANDIDATE LBVs, Fe II EMISSION LINE STARS, AND OTHER SUPERGIANTS|url=https://iopscience.iop.org/article/10.1088/0004-637X/790/1/48|journal=The Astrophysical Journal|volume=790|issue=1|page=48|arxiv=1407.2259|bibcode=2014ApJ...790...48H|doi=10.1088/0004-637X/790/1/48|issn=0004-637X|s2cid=119177378|access-date=2021-07-11|archive-date=2021-08-24|archive-url=https://web.archive.org/web/20210824142336/https://iopscience.iop.org/article/10.1088/0004-637X/790/1/48|dead-url=no}}</ref>
|-
|-
| style="background: {{star-color|O}};" |[[Sk -69° 212]] (位于[[大麦哲伦星系]]内的[[NGC 2044]])
| [[仙王座VV|仙王座VV B]]
|2377000
|  
| −7.8
| -11.2
|160000
| 100,000
|12.416
|45400
|{{SIMBAD link|Sk+-69+212|SIMBAD}}
|<ref name=":42" /><ref name=":7" />
|-
|-
| style="background: {{star-color|WC}};" |[[WR 93]] (位于[[NGC 6357]]内的[[匹斯密斯24]])
|| [[参宿三]]
|2377000
| 2.23
| −7.6
| -11.2
|5700
| 87,000
|10.68
|71000
|{{SIMBAD link|WR+93|SIMBAD}}
|<ref name="Massey et al. 2001">{{Cite journal|last1=Massey|first1=P.|last2=Degioia-Eastwood|first2=K.|last3=Waterhouse|first3=E.|year=2001|title=The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster Turnoffs. II. Results from 12 Galactic Clusters and OB Associations|url=https://archive.org/details/sim_astronomical-journal_2001-02_121_2/page/1050|journal=The Astronomical Journal|volume=121|issue=2|pages=1050–1070|arxiv=astro-ph/0010654|bibcode=2001AJ....121.1050M|doi=10.1086/318769|s2cid=53345173}}</ref><ref name="ducati" />
|-
|-
| style="background: {{star-color|WC}};" |[[BAT99-116]] B (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[弧矢二]]
|2344000
| 2.45
| −7.51
| -11.185
|163000
| 80,000
|13.09
|53000
|{{SIMBAD link|Cl*+NGC+2070+MEL+34|SIMBAD}}
|<ref name="tehrani" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[VVV CL041]]-8 (位于[[VVV CL041]])
| [[參宿七]]
|2344000
| 0.12
| −7.3
| -11.185
|13700
| 66,000
|10.146 (J波段)
|34000
|{{SIMBAD link|CRB2015+VVV+CL041-8|SIMBAD}}
|<ref>{{Cite journal|last=Chené|first=A.-N.|last2=Ramírez Alegría|first2=S.|last3=Borissova|first3=J.|last4=O’Leary|first4=E.|last5=Martins|first5=F.|last6=Hervé|first6=A.|last7=Kuhn|first7=M.|last8=Kurtev|first8=R.|last9=Consuelo Amigo Fuentes|first9=P.|last10=Bonatto|first10=C.|last11=Minniti|first11=D.|date=December 2015|title=Massive open star clusters using the VVV survey: IV. WR 62-2, a new very massive star in the core of the VVV CL041 cluster|url=http://www.aanda.org/10.1051/0004-6361/201525958|journal=Astronomy & Astrophysics|volume=584|page=A31|arxiv=1510.02539|bibcode=2015A&A...584A..31C|doi=10.1051/0004-6361/201525958|issn=0004-6361|s2cid=118707197}}</ref><ref name=":3" />
|-
|-
| style="background: {{star-color|O}};" |[[Cl 1813-178]] #16 (位于[[W33分子云]]内的[[Cl 1813-178]])
| [[参宿六]]
|2291000
| 2.07
| −7.3
| -11.16
|15300
| 66,000
|9.428 (J波段)
|30200
|{{SIMBAD link|MFD2008+16|SIMBAD}}
|<ref>{{Cite journal|last=Messineo|first=Maria|last2=Davies|first2=Ben|last3=Figer|first3=Donald F.|last4=Kudritzki|first4=R. P.|last5=Valenti|first5=Elena|last6=Trombley|first6=Christine|last7=Najarro|first7=F.|last8=Michael Rich|first8=R.|date=20 May 2011|title=Massive Stars in the Cl 1813-178 Cluster: An Episode Of Massive Star Formation in the W33 Complex|url=https://iopscience.iop.org/article/10.1088/0004-637X/733/1/41|journal=The Astrophysical Journal|volume=733|issue=1|page=41|arxiv=1103.4975|bibcode=2011ApJ...733...41M|doi=10.1088/0004-637X/733/1/41|issn=0004-637X|s2cid=118576212|access-date=2021-07-11|archive-date=2021-04-10|archive-url=https://web.archive.org/web/20210410161241/https://iopscience.iop.org/article/10.1088/0004-637X/733/1/41|dead-url=no}}</ref><ref name=":3" />
|-
|-
| style="background: {{star-color|B}};" |[[VVV CL074]]-12 (位于[[VVV CL074]])
| [[觜宿一]]
|2291000
| 3.39
| −7.3
| -11.16
|20000
| 66,000
|12.34 (J波段)
|22500
|{{SIMBAD link|CBB2013+VVV+CL074+12|SIMBAD}}
|<ref name=":11">{{Cite journal|last1=Martins|first1=F.|last2=Chené|first2=A.-N.|last3=Bouret|first3=J.-C.|last4=Borissova|first4=J.|last5=Groh|first5=J.|last6=Ramírez Alegría|first6=S.|last7=Minniti|first7=D.|date=2019|title=Massive stars in the young cluster VVV CL074|url=https://www.aanda.org/10.1051/0004-6361/201935605|journal=Astronomy & Astrophysics|volume=627|page=A170|arxiv=1907.02357|bibcode=2019A&A...627A.170M|doi=10.1051/0004-6361/201935605|issn=0004-6361|s2cid=195798873}}</ref>
|-
|-
| style="background: {{star-color|WC}};" |[[圆拱星团]]-F6 (位于[[圆拱星团]])
| [[大犬座ο1]]
|2239000
| 3.83
| −7.3
| -11.135
|25000
| 66,000
|15.75 (J波段)
|33900
|{{SIMBAD link|FNG2002+6|SIMBAD}}
|<ref name="martins">{{Cite journal|last1=Martins|first1=F.|last2=Hillier|first2=D. J.|last3=Paumard|first3=T.|last4=Eisenhauer|first4=F.|last5=Ott|first5=T.|last6=Genzel|first6=R.|date=2008|title=The most massive stars in the Arches cluster|journal=Astronomy and Astrophysics|volume=478|issue=1|pages=219–233|arxiv=0711.0657|bibcode=2008A&A...478..219M|doi=10.1051/0004-6361:20078469|s2cid=7509876}}</ref><ref name=":5" />
|-
|-
| style="background: {{star-color|WC}};" |[[圆拱星团]]-F9 (位于[[圆拱星团]])
| [[參宿四]]
|2239000
| 0.58
| −7.2
| -11.135
|25000
| 60,000
|16.1 (J波段)
|36600
|{{SIMBAD link|FNG2002+9|SIMBAD}}
|<ref name="martins" /><ref name=":5">{{Cite journal|last1=Figer|first1=Donald F.|last2=Najarro|first2=Francisco|last3=Gilmore|first3=Diane|last4=Morris|first4=Mark|last5=Kim|first5=Sungsoo S.|last6=Serabyn|first6=Eugene|last7=McLean|first7=Ian S.|last8=Gilbert|first8=Andrea M.|last9=Graham|first9=James R.|last10=Larkin|first10=James E.|last11=Levenson|first11=N. A.|date=2002-12-10|title=Massive Stars in the Arches Cluster|url=https://iopscience.iop.org/article/10.1086/344154|journal=The Astrophysical Journal|volume=581|issue=1|pages=258–275|arxiv=astro-ph/0208145|bibcode=2002ApJ...581..258F|doi=10.1086/344154|issn=0004-637X|s2cid=119002004}}</ref>
|-
|-
| style="background: {{star-color|WN}};" |[[HD 5980]] A (位于[[小麦哲伦星系]]内的[[NGC 346]])
| [[心宿二]]
|2239000
| 0.92
| −7.2
| -11.135
|200000
| 60,000
|11.31
|21000-53000
|{{SIMBAD link|HD+5980|SIMBAD}}
|<ref name="shenar">{{cite journal|last1=Shenar|first1=T.|last2=Hainich|first2=R.|last3=Todt|first3=H.|last4=Sander|first4=A.|last5=Hamann|first5=W.-R.|last6=Moffat|first6=A. F. J.|last7=Eldridge|first7=J. J.|last8=Pablo|first8=H.|last9=Oskinova|first9=L. M.|last10=Richardson|first10=N. D.|year=2016|title=Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries|journal=Astronomy & Astrophysics|volume=1604|page=A22|arxiv=1604.01022|bibcode=2016A&A...591A..22S|doi=10.1051/0004-6361/201527916|s2cid=119255408}}</ref><ref name="tycho2" />
|-
|-
| style="background: {{star-color|WC}};" |[[NGC 3603-C|HD 97950 C]]1 (位于[[NGC 3603]]内的[[HD 97950]])
| [[御夫座ψ1]]
|2239000
| 4.92
| −6.95
| -11.135
|24000
| 47,000
|11.89
|44000
|{{SIMBAD link|HD+97950C|SIMBAD}}
|<ref name="crowther" /><ref name="melena2008" />
|-
|-
| style="background: {{star-color|O}};" |[[R136b]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[弧矢一]]
|2239000
| 1.83
| −6.87
| -11.135
|165000
| 44,000
|13.24
|37000
|{{SIMBAD link|RMC136b|SIMBAD}}
|<ref name="bestenlehner2020" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[R145]] A (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[参宿增一|参宿增一A]]
|2239000
| 4.2
| −6.6
| -11.135
|163000
| 35,000
|12.04
|50000
|{{SIMBAD link|RMC145|SIMBAD}}
|<ref name="shenar2016">{{Cite journal|last1=Shenar|first1=T.|display-authors=etal|year=2016|title=The Tarantula Massive Binary Monitoring project: II. A first SB2 orbital and spectroscopic analysis for the Wolf-Rayet binary R145|journal=Astronomy & Astrophysics|volume=598|page=A85|arxiv=1610.07614|bibcode=2017A&A...598A..85S|doi=10.1051/0004-6361/201629621|s2cid=118546102}}</ref><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WN}};" |[[Var 83]] (位于[[三角座星系]])
| [[十字架三]]
|2239000
| 1.25
| −6.6
| -11.135
|3000000
| 35,000
|16.027
|18000-37000
|{{SIMBAD link|VHK+83|SIMBAD}}
|<ref name="Szeifert et al. 1996">{{Cite journal|last1=Szeifert|first1=T.|last2=Humphreys|first2=R. M.|last3=Davidson|first3=K.|last4=Jones|first4=T. J.|last5=Stahl|first5=O.|last6=Wolf|first6=B.|last7=Zickgraf|first7=F.-J.|date=1996|title=HST and groundbased observations of the 'Hubble-Sandage' variables in M 31 and M 33|url=https://archive.org/details/sim_astronomy-and-astrophysics_1996-10_314_1/page/131|journal=Astronomy and Astrophysics|volume=314|pages=131–145|bibcode=1996A&A...314..131S}}</ref><ref>{{Cite journal|last1=Massey|first1=Philip|last2=Neugent|first2=Kathryn F.|last3=Smart|first3=Brianna M.|date=2016-08-19|title=A Spectroscopic Survey of Massive Stars in M31 and M33|url=https://iopscience.iop.org/article/10.3847/0004-6256/152/3/62|journal=The Astronomical Journal|volume=152|issue=3|page=62|arxiv=1604.00112|bibcode=2016AJ....152...62M|doi=10.3847/0004-6256/152/3/62|issn=1538-3881|s2cid=35672588}}</ref>
|-
|-
| style="background: {{star-color|WC}};" |[[CXOGC J174712.2-283121]] (位于[[银心]])
| [[猎户座η]]
|2188000
| 3.38
| −6.5
| -11.11
|26000
| 32,000
|17.06 (J波段)
|35000
|{{SIMBAD link|CXOGC+J174712.2-283121|SIMBAD}}
|<ref name=":21" />
|-
|-
| style="background: {{star-color|O}};" |[[HD 269810]] (位于[[大麦哲伦星系]]内的[[NGC 2032]])
| [[大犬座ο²]]
|2188000
| 3.02
| −6.46
| -11.11
|170000
| 30,000
|12.22
|52500
|{{SIMBAD link|HD+269810|SIMBAD}}
|<ref name=":0">{{Cite journal|last1=Walborn|first1=N. R.|last2=Morrell|first2=N. I.|last3=Howarth|first3=I. D.|last4=Crowther|first4=P. A.|last5=Lennon|first5=D. J.|last6=Massey|first6=P.|last7=Arias|first7=J. I.|year=2004|title=A CNO Dichotomy among O2 Giant Spectra in the Magellanic Clouds|journal=The Astrophysical Journal|volume=608|issue=2|pages=1028–1038|arxiv=astro-ph/0403557|bibcode=2004ApJ...608.1028W|doi=10.1086/420761|s2cid=16656083}}</ref><ref name="zacharias">{{cite journal|last1=Zacharias|first1=N.|last2=Finch|first2=C. T.|last3=Girard|first3=T. M.|last4=Henden|first4=A.|last5=Bartlett|first5=J. L.|last6=Monet|first6=D. G.|last7=Zacharias|first7=M. I.|display-authors=5|date=July 2012|title=VizieR On-line Data Catalog: UCAC4 Catalogue|journal=VizieR On-line Data Catalog: I/322A|volume=1322|bibcode=2012yCat.1322....0Z}}</ref>
|-
|-
| style="background: {{star-color|O}};" |[[VFTS 1021]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[十字架二]]
|2188000
| 0.76
| −6.25
| -11.11
|164000
| 25,000
|13.35
|39800
|{{SIMBAD link|VFTS+1021|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|O}};" |[[ST5-31]] (位于[[大麦哲伦星系]]内的[[NGC 2074]])
| [[天津一]]
|2168000
| 2.23
| −6.12
| -11.1
|160000
| 22,000
|12.273
|50700
|{{SIMBAD link|ST92+5-31|SIMBAD}}
|<ref name=":42" /><ref>{{Cite journal|last1=Zaritsky|first1=Dennis|last2=Harris|first2=Jason|last3=Thompson|first3=Ian B.|last4=Grebel|first4=Eva K.|date=October 2004|title=The Magellanic Clouds Photometric Survey: The Large Magellanic Cloud Stellar Catalog and Extinction Map|url=https://iopscience.iop.org/article/10.1086/423910|journal=The Astronomical Journal|volume=128|issue=4|pages=1606–1614|arxiv=astro-ph/0407006|bibcode=2004AJ....128.1606Z|doi=10.1086/423910|issn=0004-6256|s2cid=119532934|access-date=2021-07-11|archive-date=2021-06-08|archive-url=https://web.archive.org/web/20210608170958/https://iopscience.iop.org/article/10.1086/423910|dead-url=no}}</ref>
|-
|-
| style="background: {{star-color|O}};" |[[G0.058+0.014]] (位于[[银心]])
| [[帝座]]
|2138000
| 3.48
| −5.97
| -11.085
|26000
| 19,400
|14.704 (J波段)
|45000
|{{SIMBAD link|MCD2010+G0.058%2B0.014|SIMBAD}}
|<ref name="mcd2010" />
|-
|-
| style="background: {{star-color|O}};" |[[HSH95-36]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[御夫座ε]]
|2138000
| 3.04
| −5.95
| -11.085
|163000
| 19,000
|14.41
|52000
|{{SIMBAD link|HSH95+36|SIMBAD}}
|<ref name="bestenlehner2020" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[R145]] B (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[參旗七]]
|2138000
| 3.67
| −5.8
| -11.085
|163000
| 17,000
|12.04
|43000
|{{SIMBAD link|RMC145|SIMBAD}}
|<ref name="shenar2016" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[WR 89]] (位于[[HM 1]])
| [[Iota1 Scorpii]]
|2138000
| 2.99
| −5.71
| -11.085
|9500
| 15,000
|11.02
|39800
|{{SIMBAD link|WR+89|SIMBAD}}
|<ref name="WN" /><ref name="zacharias" />
|-
|-
| style="background: {{star-color|WN}};" |[[AFGL 2298]] (靠近[[银河平面]])
| [[軒轅十三]]
|2000000
| 3.48
| −5.60
| -11.013
|33000
| 14,000
|12.164 (J波段)
|15500-26000
|{{SIMBAD link|AFGL+2298|SIMBAD}}
|<ref name="afgl2298">{{Cite journal|last1=Clark|first1=J. S.|last2=Crowther|first2=P. A.|last3=Larionov|first3=V. M.|last4=Steele|first4=I. A.|last5=Ritchie|first5=B. W.|last6=Arkharov|first6=A. A.|year=2009|title=Bolometric luminosity variations in the luminous blue variable AFGL2298|journal=Astronomy and Astrophysics|volume=507|issue=3|pages=1555–1565|arxiv=0909.4160|bibcode=2009A&A...507.1555C|doi=10.1051/0004-6361/200912358|s2cid=119187994}}</ref><ref name=":3" />
|-
|-
| style="background: {{star-color|WC}};" |[[圆拱星团]]-F1 (位于[[圆拱星团]])
| [[角宿一]]
|1995000
| 1.00
| −5.6
| -11.01
|25000
| 14,000
|16.3 (J波段)
|33200
|{{SIMBAD link|FNG2002+1|SIMBAD}}
|<ref name="martins" /><ref name=":5" />
|-
|-
| style="background: {{star-color|WC}};" |[[圆拱星团]]-F4 (位于[[圆拱星团]])
| [[海石五]]
|1995000
| 2.92
| −5.56
| -11.01
|25000
| 13,300
|15.63 (J波段)
|36800
|{{SIMBAD link|FNG2002+4|SIMBAD}}
|<ref name="martins" /><ref name=":5" />
|-
|-
| style="background: {{star-color|WC}};" |[[圆拱星团]]-F7 (位于[[圆拱星团]])
| [[老人星]]
|1995000
| −0.62
| −5.53
| -11.01
|25000
| 12,900
|15.74 (J波段)
|32900
|{{SIMBAD link|FNG2002+7|SIMBAD}}
|<ref name="martins" /><ref name=":5" />
|-
|-
| style="background: {{star-color|WC}};" |[[CXOGC J174656.3-283232]] (位于[[银心]])
| [[獵戶座ι]]
|1995000
| 2.77
| −5.5
| -11.01
|26000
| 12,600
|16.74 (J波段)
|30000
|{{SIMBAD link|CXOGC+J174656.3-283232|SIMBAD}}
|<ref name=":21" />
|-
|-
| style="background: {{star-color|WN}};" |[[LBV 1806-20]] (位于[[银心]]内的[[G10.0–0.3]])
| [[馬腹一]]
|1995000
| 0.61
| −5.42
| -11.01
|28000
| 11,700
|13.66 (J波段)
|18000-32000
|{{SIMBAD link|LBV+1806-20|SIMBAD}}
|<ref name="abdalla">{{cite journal|last1=Abdalla|first1=H.|last2=Abramowski|first2=A.|last3=Aharonian|first3=F.|last4=Ait Benkhali|first4=F.|last5=Akhperjanian|first5=A. G.|last6=Angüner|first6=E. O.|last7=Arrieta|first7=M.|last8=Aubert|first8=P.|last9=Backes|first9=M.|last10=Balzer|first10=A.|last11=Barnard|first11=M.|display-authors=29|year=2018|title=Extended VHE γ-ray emission towards SGR1806−20, LBV 1806−20, and stellar cluster Cl* 1806−20|journal=Astronomy & Astrophysics|volume=612|page=A11|arxiv=1606.05404|bibcode=2018A&A...612A..11H|doi=10.1051/0004-6361/201628695|first12=Y.|last30=Casanova|first29=J.|last29=Carr|first28=M.|last28=Capasso|first27=T.|first26=M.|last25=Brun|last26=Bryan|first25=P.|first24=F.|last27=Bulik|first18=R.|first23=J.|first16=K.|last12=Becherini|first30=S.|last16=Bernlöhr|last13=Becker Tjus|last20=Boisson|last18=Blackwell|first14=D.|last15=Bernhard|first15=S.|last17=Birsin|last23=Bregeon|first17=E.|last19=Böttcher|last24=Brun|first19=M.|first20=C.|first13=J.|last21=Bolmont|first21=J.|last22=Bordas|first22=P.|last14=Berge|s2cid=118345803}}</ref><ref name=":3" />
|-
|-
| style="background: {{star-color|WC}};" |[[默瑟81]]-2 (位于[[G338.4+0.2]]内的[[默瑟81]])
| [[廁一]]
|1995000
| 2.58
| −5.40
| -11.01
|35900
| 11,500
|13.25 (J波段)
|36000
|{{SIMBAD link|DDN2012+2|SIMBAD}}
|<ref>{{Cite journal|last=Davies|first=Ben|last2=de la Fuente|first2=Diego|last3=Najarro|first3=Francisco|last4=Hinton|first4=Jim A.|last5=Trombley|first5=Christine|last6=Figer|first6=Donald F.|last7=Puga|first7=Elena|date=21 January 2012|title=A newly discovered young massive star cluster at the far end of the Galactic Bar: A young cluster at the far end of the Bar|url=https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2011.19840.x|journal=Monthly Notices of the Royal Astronomical Society|volume=419|issue=3|pages=1860–1870|arxiv=1111.2630|bibcode=2012MNRAS.419.1860D|doi=10.1111/j.1365-2966.2011.19840.x|issn=0035-8711|s2cid=59405479}}</ref>
|-
|-
| style="background: {{star-color|WC}};" |[[VFTS 545]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[Phi Velorum]]
|1995000
| 3.52
| −5.34
| -11.01
|164000
| 10,900
|13.32
|47300
|{{SIMBAD link|VFTS+545|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[WR 147|WR 147S]] (位于[[天鹅座OB2]])
| [[天社一]]
|1995000
| 1.75
| −5.31
| -11.01
|5800
| 10,600
|13.86
|39800
|{{SIMBAD link|WR+147|SIMBAD}}
|<ref name="WN" /><ref>{{Cite journal|last1=Niemela|first1=Virpi S.|last2=Shara|first2=Michael M.|last3=Wallace|first3=Debra J.|last4=Zurek|first4=David R.|last5=Moffat|first5=Anthony F. J.|date=1998|title=Hubble Space Telescope Detection of Optical Companions of WR 86, WR 146, and WR 147: Wind Collision Model Confirmed|url=https://iopscience.iop.org/article/10.1086/300320|journal=The Astronomical Journal|volume=115|issue=5|pages=2047–2052|bibcode=1998AJ....115.2047N|doi=10.1086/300320|access-date=2021-07-11|archive-date=2020-05-29|archive-url=https://web.archive.org/web/20200529202828/https://iopscience.iop.org/article/10.1086/300320|dead-url=no}}</ref>
|-
|-
| style="background: {{star-color|WC}};" |[[DBSB 179]]-15 (位于[[G347.6+0.2]]内的[[DBSB 179]])
| [[獵戶座VV]]
|1950000
| 5.34
| −5.2
| -10.985
|25800
| 9,600
|12.5 (J波段)
|37000
|{{SIMBAD link|BIH2008+obj15|SIMBAD}}
|<ref name=":18">{{Cite journal|last=Borissova|first=J.|last2=Georgiev|first2=L.|last3=Hanson|first3=M. M.|last4=Clarke|first4=J. R. A.|last5=Kurtev|first5=R.|last6=Ivanov|first6=V. D.|last7=Penaloza|first7=F.|last8=Hillier|first8=D. J.|last9=Zsargó|first9=J.|date=October 2012|title=Obscured clusters: IV. The most massive stars in [DBS2003] 179|url=http://www.aanda.org/10.1051/0004-6361/201118348|journal=Astronomy & Astrophysics|volume=546|page=A110|arxiv=1209.6370|bibcode=2012A&A...546A.110B|doi=10.1051/0004-6361/201118348|issn=0004-6361|s2cid=119303823}}</ref><ref name=":19">{{Cite journal|last=Borissova|first=J.|last2=Ivanov|first2=V. D.|last3=Hanson|first3=M. M.|last4=Georgiev|first4=L.|last5=Minniti|first5=D.|last6=Kurtev|first6=R.|last7=Geisler|first7=D.|date=September 2008|title=The young Galactic star cluster [DBS2003] 179|url=http://www.aanda.org/10.1051/0004-6361:20079255|journal=Astronomy & Astrophysics|volume=488|issue=1|pages=151–159|arxiv=0806.4584|bibcode=2008A&A...488..151B|doi=10.1051/0004-6361:20079255|issn=0004-6361|s2cid=14942349}}</ref>
|-
|-
| style="background: {{star-color|WC}};" |[[G0.114+0.021]] (位于[[银心]])
| [[尾宿八]]
|1950000
| 1.62
| −5.05
| -10.985
|26000
| 8,400
|16.672 (J波段)
|40000
|{{SIMBAD link|MCD2010+G0.114%2B0.021|SIMBAD}}
|<ref name="mcd2010" />
|-
|-
| style="background: {{star-color|O}};" |[[R136a5]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[弧矢九]]
|1950000
| 2.71
| −4.92
| -10.985
|165000
| 7,400
|13.71
|47000
|{{SIMBAD link|RMC136a5|SIMBAD}}
|<ref name="bestenlehner2020" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[AB6]] A (位于[[小麦哲伦星系]]内的[[NGC 371]])
| [[危宿三]]
|1905000
| 2.38
| −4.8
| -10.96
|197000
| 6,600
|12.3
|80000
|{{SIMBAD link|SMC+AB+6|SIMBAD}}
|<ref name="shenar" /><ref name=":6">{{Cite journal|last1=Bonanos|first1=A. Z.|last2=Lennon|first2=D. J.|last3=Köhlinger|first3=F.|last4=van Loon|first4=J. Th.|last5=Massa|first5=D. L.|last6=Sewilo|first6=M.|last7=Evans|first7=C. J.|last8=Panagia|first8=N.|last9=Babler|first9=B. L.|last10=Block|first10=M.|last11=Bracker|first11=S.|date=2010-08-01|title=Spitzersage-SMC Infrared Photometry of Massive Stars in the Small Magellanic Cloud|url=https://iopscience.iop.org/article/10.1088/0004-6256/140/2/416|journal=The Astronomical Journal|volume=140|issue=2|pages=416–429|arxiv=1004.0949|bibcode=2010AJ....140..416B|doi=10.1088/0004-6256/140/2/416|issn=0004-6256|s2cid=119290443|access-date=2021-07-11|archive-date=2021-06-06|archive-url=https://web.archive.org/web/20210606104955/https://iopscience.iop.org/article/10.1088/0004-6256/140/2/416|dead-url=no}}</ref>
|-
|-
| style="background: {{star-color|O}};" |[[R136a8]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[弧矢七]]
|1905000
| 1.50
| −4.8
| -10.96
|165000
| 6,600
|14.42
|51000
|{{SIMBAD link|RMC136a8|SIMBAD}}
|<ref name="crowther2016">{{cite journal|last1=Crowther|first1=Paul A.|last2=Caballero-Nieves|first2=S. M.|last3=Bostroem|first3=K. A.|last4=Maíz Apellániz|first4=J.|last5=Schneider|first5=F. R. N.|last6=Walborn|first6=N. R.|last7=Angus|first7=C. R.|last8=Brott|first8=I.|last9=Bonanos|first9=A.|last10=De Koter|first10=A.|last11=De Mink|first11=S. E.|year=2016|title=The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of He II λ1640 in young star clusters|journal=Monthly Notices of the Royal Astronomical Society|volume=458|issue=1|pages=624–659|arxiv=1603.04994|bibcode=2016MNRAS.458..624C|doi=10.1093/mnras/stw273|last18=Puls|first16=N.|last13=Gräfener|first13=G.|last14=Herrero|first14=A.|last15=Howarth|first15=I. D.|first18=J.|first12=C. J.|last16=Langer|last19=Sana|first19=H.|last20=Vink|first20=J. S.|author11-link=Selma de Mink|first17=D. J.|last12=Evans|last17=Lennon}}</ref><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[WR 22]] A (位于[[船底座星云]]的[[波鸿10]])
| [[参宿五]]
|1905000
| 1.64
| −4.75
| -10.96
|8200
| 6,300
| style="background: lightblue;" |6.42
|44700
|{{SIMBAD link|WR+22|SIMBAD}}
|<ref name="WN" /><ref name="ducati" />
|-
|-
| style="background: {{star-color|O}};" |[[R136a6]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[Xi Puppis]]
|1862000
| 3.34
| −4.74
| -10.935
|165000
| 6,250
|13.35
|53000
|{{SIMBAD link|RMC136a6|SIMBAD}}
|<ref name="bestenlehner2020" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[Hen 3-519]] (位于[[蓝泡泡星云]])
| [[海石一]]
|1820000
| 1.86
| −4.58
| -10.91
|24000
| 5,400
|10.85
|30200
|{{SIMBAD link|Hen+3-519|SIMBAD}}
|<ref name="vangenderen">{{cite journal|last1=Van Genderen|first1=A. M.|year=2001|title=S Doradus variables in the Galaxy and the Magellanic Clouds|journal=Astronomy and Astrophysics|volume=366|issue=2|pages=508–531|bibcode=2001A&A...366..508V|doi=10.1051/0004-6361:20000022|doi-access=free}}[http://vizier.cfa.harvard.edu/viz-bin/VizieR-6?-out.form=%2bH&-source=33660508&-out.all&-corr=PFK=Name&-out.max=9999&Name==He3-519 Vizie database entry] {{Wayback|url=http://vizier.cfa.harvard.edu/viz-bin/VizieR-6?-out.form=%2bH&-source=33660508&-out.all&-corr=PFK=Name&-out.max=9999&Name==He3-519 |date=20210205041313 }}</ref><ref name="tycho2">{{cite journal|last1=Høg|first1=E.|last2=Fabricius|first2=C.|last3=Makarov|first3=V. V.|last4=Urban|first4=S.|last5=Corbin|first5=T.|last6=Wycoff|first6=G.|last7=Bastian|first7=U.|last8=Schwekendiek|first8=P.|last9=Wicenec|first9=A.|year=2000|title=The Tycho-2 catalogue of the 2.5 million brightest stars|journal=Astronomy and Astrophysics|volume=355|page=L27|bibcode=2000A&A...355L..27H|doi=10.1888/0333750888/2862|isbn=0333750888}}</ref>
|-
|-
| style="background: {{star-color|WN}};" |[[LGGS J004051.59+403303.0]] (位于[[仙女座星系]])
| [[獵戶座W]]
|1803000
| 5.88
| −4.4
| -10.9
|2500000
| 4,600
|16.989
|18000-24000
|{{SIMBAD link|LGGS+J004051.59%2B403303.0|SIMBAD}}
|<ref name="m31" /><ref name=":4" />
|-
|-
| style="background: {{star-color|WN}};" |[[Wray 17-96|MSX5C G358.5391+00.1305]] (位于[[Wray 17-96]])
| [[水委一]]
|1800000
| 0.46
| −4.05
| -10.898
|15000
| 3,300[http://arxiv.org/abs/astro-ph/0602084]
|15
|13000
|{{SIMBAD link|MSX5C+G358.5391%2B00.1305|SIMBAD}}
|<ref name="egan">{{Cite journal|last=Egan|first=Michael P.|display-authors=etal|year=2002|title=An Infrared Ring Nebula around MSX5C G358.5391+00.1305: The True Nature of Suspected Planetary Nebula Wray 17-96 Determined via Direct Imaging and Spectroscopy|journal=The Astrophysical Journal|volume=572|issue=1|pages=288–299|bibcode=2002ApJ...572..288E|doi=10.1086/340222|doi-access=free}}</ref><ref name="zacharias" />
|-
|-
| style="background: {{star-color|WC}};" |[[HD 5980]] B (位于[[小麦哲伦星系]]内的[[NGC 346]])
| [[天琴座β]]
|1778000
| 3.52
| −3.91
| -10.885
|200000
| 2,900
|11.31
|45000
|{{SIMBAD link|HD+5980|SIMBAD}}
|<ref name="shenar" /><ref name="melena2008" />
|-
|-
| style="background: {{star-color|O}};" |[[R136a7]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[勾陳一]]
|1778000
| 1.97
| −3.6
| -10.885
|165000
| 2,200
|13.97
|49000
|{{SIMBAD link|RMC136a7|SIMBAD}}
|<ref name="bestenlehner2020" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[WR 130]] (位于[[天鹅座OB3]])
| [[十字架一]]
|1778000
| 1.63
| −3.2
| -10.885
|21700
| 1,500
|12.13
|44700
|{{SIMBAD link|WR+130|SIMBAD}}
|<ref name="WN" /><ref name="zacharias" />
|-
|-
| style="background: {{star-color|WC}};" |[[WR 21a]] A (来自[[维斯特卢2]]的[[速逃星]])
| [[軒轅十四]]
|1778000
| 1.35
| −1.6
| -10.885
|14300
| 350[http://spider.ipac.caltech.edu/staff/gerard/postscript/mcalister+_2005.pdf]
|12.661
|45000
|{{SIMBAD link|WR+21a|SIMBAD}}
|<ref name="tramper">{{cite journal|last1=Tramper|first1=F.|last2=Sana|first2=H.|last3=Fitzsimons|first3=N. E.|last4=De Koter|first4=A.|last5=Kaper|first5=L.|last6=Mahy|first6=L.|last7=Moffat|first7=A.|year=2016|title=The mass of the very massive binary WR21a|journal=Monthly Notices of the Royal Astronomical Society|volume=455|issue=2|pages=1275–1281|arxiv=1510.03609|bibcode=2016MNRAS.455.1275T|doi=10.1093/mnras/stv2373|s2cid=44364798}}</ref><ref name="zacharias" />
|-
|-
| style="background: {{star-color|WN}};" |[[人马座V4650]] (位于[[五合星团]])
| [[畢宿五]]
|1770000
| 0.85
| −0.63
| -10.88
|25000
| 140
|12.31 (J波段)
|11300
|{{SIMBAD link|V4650+Sagittarii|SIMBAD}}
|<ref>{{Cite journal|last1=Najarro|first1=F.|last2=Figer|first2=D. F.|last3=Hillier|first3=D. J.|last4=Geballe|first4=T. R.|last5=Kudritzki|first5=R. P.|year=2009|title=Metallicity in the Galactic Center: The Quintuplet Cluster|journal=The Astrophysical Journal|volume=691|issue=2|pages=1816–1827|arxiv=0809.3185|bibcode=2009ApJ...691.1816N|doi=10.1088/0004-637X/691/2/1816|s2cid=15473563}}</ref><ref name="qc" />
|-
|-
| style="background: {{star-color|WC}};" |[[CXOGC J174536.1-285638]] (位于[[银心]])
| [[大角星]]
|1738000
| −0.04
| −0.31
| -10.86
|26000
| 110
|15.55 (J波段)
|30000
|{{SIMBAD link|CXOGC+J174536.1-285638|SIMBAD}}
|<ref name=":21" />
|-
|-
| style="background: {{star-color|WC}};" |[[默瑟30]]-7 A (位于[[龙鱼星云]]内的[[默瑟30]])
| [[五車二]]
|1738000
| 0.08
| 0.4
| -10.86
|40000
| 55
|11.516 (J波段)
|41400
|{{SIMBAD link|DNB2016+Mc30-7|SIMBAD}}
|<ref name=":17" />
|-
|-
| style="background: {{star-color|O}};" |[[R136a4]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[北河二]]
|1738000
| 1.98
| 0.5
| -10.86
|165000
| 50
|13.41
|48000
|{{SIMBAD link|RMC136a4|SIMBAD}}
|<ref name="bestenlehner2020" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|O}};" |[[VFTS 506]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[織女一]]
|1738000
| 0.00
| 0.58
| -10.86
|164000
| 47
|13.31
|47300
|{{SIMBAD link|VFTS+506|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|WC}};" |[[DBSB 179]]-20 (位于[[G347.6+0.2]]内的[[DBSB 179]])
| [[北河三]]
|1698000
| 1.14
| 0.7
| -10.835
|25800
| 42
|12.37 (J波段)
|35000
|{{SIMBAD link|BIH2008+obj20|SIMBAD}}
|<ref name=":18" /><ref name=":19" />
|-
|-
| style="background: {{star-color|WC}};" |[[R147]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[天狼星]]
|1698000
| −1.46
| 1.4
| -10.835
|164000
| 22
|13.02
|50000
|{{SIMBAD link|RMC147|SIMBAD}}
|<ref name="hainich" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|O}};" |[[VFTS 16]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
| [[HD 38529]]
|1698000
| 5.94
| 2.7
| -10.835
|164000
| 6.6
|13.55
|53100
|{{SIMBAD link|VFTS+16|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
|-
| style="background: {{star-color|B}};" |[[天鹅座OB2-12]] A (位于[[天鹅座OB2]])
| [[Pi3 Orionis|Tabit]]
|1660000
| 3.19
| 3.7
| -10.81
|5000
| 2.6
|11.702
|13700
|{{SIMBAD link|Cyg+OB2+12|SIMBAD}}
|<ref name="oskinova">{{cite journal|last1=Oskinova|first1=L. M.|last2=Huenemoerder|first2=D. P.|last3=Hamann|first3=W. -R.|last4=Shenar|first4=T.|last5=Sander|first5=A. A. C.|last6=Ignace|first6=R.|last7=Todt|first7=H.|last8=Hainich|first8=R.|year=2017|title=On the Binary Nature of Massive Blue Hypergiants: High-resolution X-Ray Spectroscopy Suggests That Cyg OB2 12 is a Colliding Wind Binary|journal=The Astrophysical Journal|volume=845|issue=1|page=39|arxiv=1707.04473|bibcode=2017ApJ...845...39O|doi=10.3847/1538-4357/aa7e79|s2cid=119537489}}</ref><ref name=":9">{{Cite journal|last1=Laur|first1=Jaan|last2=Kolka|first2=Indrek|last3=Eenmäe|first3=Tõnis|last4=Tuvikene|first4=Taavi|last5=Leedjärv|first5=Laurits|date=2017|title=Variability survey of brightest stars in selected OB associations|url=http://www.aanda.org/10.1051/0004-6361/201629395|journal=Astronomy & Astrophysics|volume=598|page=A108|arxiv=1611.02452|bibcode=2017A&A...598A.108L|doi=10.1051/0004-6361/201629395|issn=0004-6361|s2cid=119076598}}</ref>
|-
|-
| style="background: {{star-color|O}};" |[[Sher 18]] (位于[[NGC 3603]]内的[[HD 97950]])
| [[南門二|半人馬座A]]
|1644000
| −0.01
| 4.38
| -10.8
|25000
| 1.4
|12.51
|39500
|{{SIMBAD link|Cl*+NGC+3603+Sher+18|SIMBAD}}
|<ref name="melena2008" /><ref name=":16">{{Cite journal|last=Moffat|first=A. F. J.|date=October 1974|title=On the distance and reddening of the massive H II region NGC 3603|url=https://ui.adsabs.harvard.edu/abs/1974A%26A....35..315M/abstract|journal=Astronomy and Astrophysics|volume=35|page=315|bibcode=1974A&A....35..315M|issn=0004-6361|s2cid=115549707}}</ref>
|-
|-
| style="background: {{star-color|O}};" |[[Sher 47]] (位于[[NGC 3603]]内的[[HD 97950]])
| [[獵戶座χ1]]
|1644000
| 4.41
| 4.7
| -10.8
|25000
| 1.05
|12.67
|44000
|{{SIMBAD link|Cl*+NGC+3603+Sher+47|SIMBAD}}
|<ref name="melena2008" /><ref name=":16" />
|-
|-
| style="background: {{star-color|O}};" |[[Mercer 23]]-1 (位于靠近[[银河平面]]的[[默瑟23]])
| [[太陽]]
|1622000
| −26.8
| 4.75
| -10.785
|21200
| 1.00
|10.615 (J波段)
|35000
|{{SIMBAD link|HKB2010b+Obj1|SIMBAD}}
|<ref name=":20" /><ref name=":3" />
|-
| style="background: {{star-color|WC}};" |[[VFTS 1017]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1622000
| -10.785
|164000
|14.52
|50100
|{{SIMBAD link|VFTS+1017|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
| style="background: {{star-color|WC}};" |[[WR 87]] (位于[[HM 1]])
|1622000
| -10.785
|9500
|11.83
|44700
|{{SIMBAD link|WR+87|SIMBAD}}
|<ref name="WN" /><ref name="zacharias" />
|-
| style="background: {{star-color|WN}};" |[[仙女座AF]] (位于[[仙女座星系]])
|1585000
| -10.76
|2500000
|17.325
|28000
|{{SIMBAD link|AF+Andromedae|SIMBAD}}
|<ref name="Szeifert et al. 1996" /><ref name=":4" />
|-
| style="background: {{star-color|WC}};" |[[圆拱星团]]-F12 (位于[[圆拱星团]])
|1585000
| -10.76
|25000
|16.4 (J波段)
|36900
|{{SIMBAD link|FNG2002+12|SIMBAD}}
|<ref name="martins" /><ref name=":5" />
|-
| style="background: {{star-color|O}};" |[[HSH95-18]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1585000
| -10.76
|163000
|13.87
|47000
|{{SIMBAD link|HSH95+18|SIMBAD}}
|<ref name="Doran2013" />
|-
| style="background: {{star-color|WC}};" |[[五合星团|LHO 110]] (位于[[五合星团]])
|1585000
| -10.76
|26000
|13.87 (J波段)
|25100
|{{SIMBAD link|LHO+110|SIMBAD}}
|<ref name="quintuplet" /><ref name="qc" />
|-
| style="background: {{star-color|WC}};" |[[R140a1]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1585000
| -10.76
|163000
|12.12
|34000
|{{SIMBAD link|RMC140a1|SIMBAD}}
|<ref name="Doran2013" />
|-
| style="background: {{star-color|WC}};" |[[VFTS 457]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1585000
| -10.76
|164000
|13.74
|39800
|{{SIMBAD link|VFTS+457|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
| style="background: {{star-color|WC}};" |[[WR 107]] (位于[[人马座OB1]])
|1585000
| -10.76
|9400
|13.51
|50100
|{{SIMBAD link|WR+107|SIMBAD}}
|<ref name="WN" /><ref name="zacharias" />
|-
| style="background: {{star-color|O}};" |[[WR 140]] B (位于[[天鹅座OB1]])
|1585000
| -10.76
|5300
|6.85
|35000
|{{SIMBAD link|WR+140|SIMBAD}}
|<ref>{{Cite journal|last=Williams|first=Peredur|date=2011|title=Results from the 2009 campaign on WR 140|journal=Société Royale des Sciences de Liège|volume=80|pages=595–609|bibcode=2011BSRSL..80..595W}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|WC}};" |[[WR 148]] A (来自[[银河平面]]的[[速逃星]])
|1585000
| -10.76
|27100
|10.3
|39800
|{{SIMBAD link|WR+148|SIMBAD}}
|<ref name="WN" /><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[CXOGC J174617.0-285131]] (位于[[银心]])
|1549000
| -10.735
|26000
|14.98 (J波段)
|40000
|{{SIMBAD link|CXOGC+J174617.0-285131|SIMBAD}}
|<ref name=":21" />
|-
| style="background: {{star-color|O}};" |[[CXOGC J174725.3-282709]] (位于[[银心]])
|1549000
| -10.735
|26000
|16.37 (J波段)
|30000
|{{SIMBAD link|CXOGC+J174725.3-282709|SIMBAD}}
|<ref name=":21" />
|-
| style="background: {{star-color|O}};" |[[Sk -68° 137]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1549000
| -10.735
|160000
|13.346
|55000
|{{SIMBAD link|Sk+-68+137|SIMBAD}}
|<ref name=":0" /><ref name=":7">{{Cite journal|last1=Bonanos|first1=A. Z.|last2=Massa|first2=D. L.|last3=Sewilo|first3=M.|last4=Lennon|first4=D. J.|last5=Panagia|first5=N.|last6=Smith|first6=L. J.|last7=Meixner|first7=M.|last8=Babler|first8=B. L.|last9=Bracker|first9=S.|last10=Meade|first10=M. R.|last11=Gordon|first11=K. D.|date=2009-10-01|title=Spitzersage Infrared Photometry of Massive Stars in the Large Magellanic Cloud|url=https://iopscience.iop.org/article/10.1088/0004-6256/138/4/1003|journal=The Astronomical Journal|volume=138|issue=4|pages=1003–1021|arxiv=0905.1328|bibcode=2009AJ....138.1003B|doi=10.1088/0004-6256/138/4/1003|issn=0004-6256|s2cid=14056495|access-date=2021-07-11|archive-date=2020-12-05|archive-url=https://web.archive.org/web/20201205083437/https://iopscience.iop.org/article/10.1088/0004-6256/138/4/1003|dead-url=no}}</ref>
|-
| style="background: {{star-color|WC}};" |[[五合星团|WR 102i]] (位于[[五合星团]])
|1549000
| -10.735
|26000
|14.31 (J波段)
|31600
|{{SIMBAD link|WR+102i|SIMBAD}}
|<ref name="quintuplet" /><ref name="qc" />
|-
| style="background: {{star-color|WC}};" |[[NGC 3603-A1|HD 97950 A1b]] (位于[[NGC 3603]]内的[[HD 97950]])
|1514000
| -10.71
|24000
|11.18
|40000
|{{SIMBAD link|Cl*+NGC+3603+BLW+A1|SIMBAD}}
|<ref name="crowther" /><ref name="melena2008" />
|-
| style="background: {{star-color|WC}};" |[[布雷21]] A (位于[[大麦哲伦星系]]内的[[NGC 1910]])
|1500000
| -10.7
|165000
|11.29
|71000
|{{SIMBAD link|Brey+21|SIMBAD}}
|<ref name=":42" /><ref name="zacharias" />
|-
| style="background: {{star-color|O}};" |[[HD 97950]] A2 (位于[[NGC 3603]]内的[[HD 97950]])
|1500000
| -10.7
|24000
|12.53
|46500
|{{SIMBAD link|Cl*+NGC+3603+BLW+A2|SIMBAD}}
|<ref name="melena2008" /><ref name=":16" />
|-
| style="background: {{star-color|O}};" |[[HM 1]]-6 (位于[[HM 1]])
|1500000
| -10.7
|11000
|11.64
|44700
|{{SIMBAD link|Cl+HM+1+6|SIMBAD}}
|<ref name="Massey et al. 2001" /><ref name=":8">{{Cite journal|last=Reed|first=B. Cameron|date=2003|title=Catalog of Galactic OB Stars|url=https://iopscience.iop.org/article/10.1086/374771|journal=The Astronomical Journal|volume=125|issue=5|pages=2531–2533|bibcode=2003AJ....125.2531R|doi=10.1086/374771|issn=0004-6256|access-date=2021-07-11|archive-date=2021-05-16|archive-url=https://web.archive.org/web/20210516115320/https://iopscience.iop.org/article/10.1086/374771|dead-url=no}}</ref>
|-
| style="background: {{star-color|O}};" |[[LGGS J013245.41+303858.3]] (位于[[三角座星系]])
|1500000
| -10.7
|3000000
|17.612
|34000
|{{SIMBAD link|LGGS+J013245.41%2B303858.3|SIMBAD}}
|<ref name="humphreys2017">{{Cite journal|last1=Humphreys|first1=Roberta M.|last2=Davidson|first2=Kris|last3=Hahn|first3=David|last4=Martin|first4=John C.|last5=Weis|first5=Kerstin|date=2017-07-06|title=Luminous and Variable Stars in M31 and M33 V. The Upper HR Diagram|journal=The Astrophysical Journal|volume=844|issue=1|page=40|arxiv=1707.01916|bibcode=2017ApJ...844...40H|doi=10.3847/1538-4357/aa7cef|s2cid=119357524}}</ref><ref name=":4" />
|-
| style="background: {{star-color|O}};" |[[NGC 346]]-W1 (位于[[小麦哲伦星系]]内的[[NGC 346]])
|1500000
| -10.7
|200000
|12.57
|43400
|{{SIMBAD link|Cl*+NGC+346+W+1|SIMBAD}}
|<ref name=":42" /><ref name=":6" />
|-
| style="background: {{star-color|O}};" |[[Sk -65° 47]] (位于[[大麦哲伦星系]]内的[[NGC 1923]])
|1500000
| -10.7
|160000
|12.466
|47800
|{{SIMBAD link|Sk+-65+47|SIMBAD}}
|<ref name=":42" /><ref name=":7" />
|-
| style="background: {{star-color|O}};" |[[Sk 80]] (位于[[小麦哲伦星系]]内的[[NGC 346]])
|1500000
| -10.7
|200000
|12.31
|38900
|{{SIMBAD link|Sk+80|SIMBAD}}
|<ref name=":42" /><ref>{{Cite journal|last1=Evans|first1=C. J.|last2=Lennon|first2=D. J.|last3=Smartt|first3=S. J.|last4=Trundle|first4=C.|date=September 2006|title=The VLT-FLAMES survey of massive stars: observations centered on the Magellanic Cloud clusters NGC 330, NGC 346, NGC 2004, and the N11 region|url=http://www.aanda.org/10.1051/0004-6361:20064988|journal=Astronomy & Astrophysics|volume=456|issue=2|pages=623–638|arxiv=astro-ph/0606405|bibcode=2006A&A...456..623E|doi=10.1051/0004-6361:20064988|issn=0004-6361|s2cid=13160849}}</ref>
|-
| style="background: {{star-color|O}};" |[[HD 93129]] Aa (位于[[船底座星云]]内的[[川普勒14]])
|1479000
| -10.685
|7500
|6.9
|42500
|{{SIMBAD link|HD+93129A|SIMBAD}}
|<ref name="smith">{{cite journal|last1=Smith|first1=Nathan|year=2006|title=A census of the Carina Nebula - I. Cumulative energy input from massive stars|journal=Monthly Notices of the Royal Astronomical Society|volume=367|issue=2|pages=763–772|arxiv=astro-ph/0601060|bibcode=2006MNRAS.367..763S|doi=10.1111/j.1365-2966.2006.10007.x|s2cid=14060690}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[HSH95-46]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1445000
| -10.66
|163000
|14.56
|49000
|{{SIMBAD link|HSH95+46|SIMBAD}}
|<ref name="bestenlehner2020" /><ref name="Doran2013" />
|-
| style="background: {{star-color|WC}};" |[[VFTS 542]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1445000
| -10.66
|164000
|13.49
|44700
|{{SIMBAD link|VFTS+542|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
| style="background: {{star-color|WC}};" |[[AB8]] A (位于[[小麦哲伦星系]]内的[[NGC 602]])
|1413000
| -10.635
|197000
|12.9
|141000
|{{SIMBAD link|SMC+AB+8|SIMBAD}}
|<ref name="shenar" /><ref>{{Cite journal|last=Massey|first=Philip|date=July 2002|title=A UBVR CCD Survey of the Magellanic Clouds|url=https://iopscience.iop.org/article/10.1086/338286|journal=The Astrophysical Journal Supplement Series|volume=141|issue=1|pages=81–122|arxiv=astro-ph/0110531|bibcode=2002ApJS..141...81M|doi=10.1086/338286|issn=0067-0049|s2cid=119447348|access-date=2021-07-11|archive-date=2021-07-11|archive-url=https://web.archive.org/web/20210711175139/https://iopscience.iop.org/article/10.1086/338286|dead-url=no}}</ref>
|-
| style="background: {{star-color|O}};" |[[圆拱星团]]-F15 (位于[[圆拱星团]])
|1413000
| -10.635
|25000
|16.12 (J波段)
|35600
|{{SIMBAD link|FNG2002+15|SIMBAD}}
|<ref name="martins" /><ref name=":5" />
|-
| style="background: {{star-color|WC}};" |[[CXOGC J174550.2-284911]] (位于[[银心]])
|1413000
| -10.635
|26000
|15.24 (J波段)
|30000
|{{SIMBAD link|CXOGC+J174550.2-284911|SIMBAD}}
|<ref name=":21" />
|-
| style="background: {{star-color|WC}};" |[[DBSB 179]]-4 (位于[[G347.6+0.2]]内的[[DBSB 179]])
|1413000
| -10.635
|25800
|12.25 (J波段)
|30000
|{{SIMBAD link|BIH2008+obj4|SIMBAD}}
|<ref name=":18" /><ref name=":19" />
|-
| style="background: {{star-color|O}};" |[[LGGS J013235.25+303017.6]] (位于[[三角座星系]])
|1413000
| -10.635
|3000000
|18.007
|33000
|{{SIMBAD link|LGGS+J013235.25%2B303017.6|SIMBAD}}
|<ref name=":2" /><ref>{{Cite journal|last1=Massey|first1=Philip|last2=Olsen|first2=K. A. G.|last3=Hodge|first3=Paul W.|last4=Jacoby|first4=George H.|last5=McNeill|first5=Reagin T.|last6=Smith|first6=R. C.|last7=Strong|first7=Shay B.|date=2007|title=A Survey of Local Group Galaxies Currently Forming Stars. II. UBVRI Photometry of Stars in Seven Dwarfs and a Comparison of the Entire Sample|url=https://iopscience.iop.org/article/10.1086/513319|journal=The Astronomical Journal|volume=133|issue=5|pages=2393–2417|arxiv=astro-ph/0702236|bibcode=2007AJ....133.2393M|doi=10.1086/513319|issn=0004-6256|s2cid=119456878}}</ref>
|-
| style="background: {{star-color|WC}};" |[[R134]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1413000
| -10.635
|164000
|12.58
|47000
|{{SIMBAD link|RMC134|SIMBAD}}
|<ref name="hainich" /><ref name="Doran2013" />
|-
| style="background: {{star-color|WN}};" |[[剑鱼座S]] (位于[[大麦哲伦星系]]内的[[NGC 1910]])
|1413000
| -10.635
|169000
|10.25
|20000
|{{SIMBAD link|S+Doradus|SIMBAD}}
|<ref name="lamers1995">{{cite conference|last=Lamers|first=H. J. G. L. M.|date=February 6–10, 1995|title=Proceedings of IAU Colloquium 155, Astrophysical applications of stellar pulsation|location=Cape Town, South Africa|publisher=Astronomical Society of the Pacific|volume=83|pages=176–191|bibcode=1995ASPC...83..176L|contribution=Observations and Interpretation of Luminous Blue Variables|journal=Astrophysical Applications of Stellar Pulsation. Astronomical Society of the Pacific Conference Series}}</ref><ref name="zacharias" />
|-
| style="background: {{star-color|WC}};" |[[WR 66]] (位于[[圆规座OB1]])
|1413000
| -10.635
|16900
|11.34
|44700
|{{SIMBAD link|WR+66|SIMBAD}}
|<ref name="WN" /><ref name="ducati" />
|-
| style="background: {{star-color|WN}};" |[[HD 37974]] (位于[[大麦哲伦星系]]内的[[N135]])
|1400000
| -10.625
|163000
|10.99
|22500
|{{SIMBAD link|HD+37974|SIMBAD}}
|<ref name="kastner">{{Cite journal|last1=Kastner|first1=J. H.|last2=Buchanan|first2=C. L.|last3=Sargent|first3=B.|last4=Forrest|first4=W. J.|year=2006|title=SpitzerSpectroscopy of Dusty Disks around B\e] Hypergiants in the Large Magellanic Cloud|journal=The Astrophysical Journal|volume=638|issue=1|pages=L29–L32|bibcode=2006ApJ...638L..29K|doi=10.1086/500804|doi-access=free}}</ref><ref name="zacharias" />
|-
| style="background: {{star-color|O}};" |[[VFTS 621]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1380000
| -10.61
|164000
|15.39
|54000
|{{SIMBAD link|VFTS+621|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
| style="background: {{star-color|WC}};" |[[WR 131]] (位于[[天鹅座OB3]])
|1380000
| -10.61
|22600
|12.08
|44700
|{{SIMBAD link|WR+131|SIMBAD}}
|<ref name="WN" /><ref name=":8" />
|-
| style="background: {{star-color|O}};" |[[Sk -69° 104]] (位于[[大麦哲伦星系]]内的[[NGC 1910]])
|1368000
| -10.6
|160000
|12.1
|39900
|{{SIMBAD link|Sk+-69+104|SIMBAD}}
|<ref name=":42" /><ref name=":7" />
|-
| style="background: {{star-color|WC}};" |[[默瑟30]]-6a A (位于[[龙鱼星云]]内的[[默瑟30]])
|1349000
| -10.585
|40000
|10.39 (J波段)
|29900
|{{SIMBAD link|DNB2016+Mc30-6a|SIMBAD}}
|<ref name=":17" />
|-
| style="background: {{star-color|WC}};" |[[VFTS 427]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1349000
| -10.585
|164000
|13.76
|39800
|{{SIMBAD link|VFTS+427|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[CXOGC J174502.8-290859]] (位于[[银心]])
|1318000
| -10.56
|26000
|13.93 (J波段)
|33000
|{{SIMBAD link|CXOGC+J174502.8-290859|SIMBAD}}
|<ref name=":21" />
|-
| style="background: {{star-color|WC}};" |[[WR 18]] (位于[[船底座星云]]内的[[船底座OB1]])
|1288000
| -10.535
|12450
|10.83
|112200
|{{SIMBAD link|WR+18|SIMBAD}}
|<ref name="WN" /><ref name="zacharias" />
|-
| style="background: {{star-color|WC}};" |[[AB7]] A (位于[[小麦哲伦星系]]内的[[NGC 371]])
|1259000
| -10.51
|197000
|13.016
|105000
|{{SIMBAD link|SMC+AB+7|SIMBAD}}
|<ref name="shenar" /><ref name=":6" />
|-
| style="background: {{star-color|WC}};" |[[圆拱星团]]-F3 (位于[[圆拱星团]])
|1259000
| -10.51
|25000
|16.06 (J波段)
|29600
|{{SIMBAD link|FNG2002+3|SIMBAD}}
|<ref name="martins" /><ref name=":5" />
|-
| style="background: {{star-color|WC}};" |[[圆拱星团]]-F8 (位于[[圆拱星团]])
|1259000
| -10.51
|25000
|16.31 (J波段)
|32900
|{{SIMBAD link|FNG2002+8|SIMBAD}}
|<ref name="martins" /><ref name=":5" />
|-
| style="background: {{star-color|WN}};" |[[HD 50064]] (位于[[NGC 2301]])
|1259000
| -10.51
|9500
|8.21
|13500
|{{SIMBAD link|HD+50064|SIMBAD}}
|<ref name="aerts">{{Cite journal|last1=Aerts|first1=C.|last2=Lefever|first2=K.|last3=Baglin|first3=A.|last4=Degroote|first4=P.|last5=Oreiro|first5=R.|last6=Vučković|first6=M.|last7=Smolders|first7=K.|last8=Acke|first8=B.|last9=Verhoelst|first9=T.|last10=Desmet|first10=M.|last11=Godart|first11=M.|date=April 2010|title=Periodic mass-loss episodes due to an oscillation mode with variable amplitude in the hot supergiant HD 50064|journal=Astronomy and Astrophysics|volume=513|page=L11|arxiv=1003.5551|bibcode=2010A&A...513L..11A|doi=10.1051/0004-6361/201014124|last14=Auvergne|last16=Catala|first18=R.|last18=Samadi|first17=E.|first16=C.|first13=M.-A.|first15=F.|last17=Michel|first14=M.|last13=Dupret|first12=A.|last12=Noels|last15=Baudin|s2cid=41541073}}</ref>
|-
| style="background: {{star-color|O}};" |[[HSH95-16]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1259000
| -10.51
|163000
|13.65
|42000
|{{SIMBAD link|HSH95+16|SIMBAD}}
|<ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[HSH95-20]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1259000
| -10.51
|164000
|13.71
|46000
|{{SIMBAD link|HSH95+20|SIMBAD}}
|<ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[R139]] A (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1259000
| -10.51
|163000
|11.94
|34000
|{{SIMBAD link|RMC139|SIMBAD}}
|<ref>{{Cite journal|last1=Taylor|first1=W. D.|last2=Evans|first2=C. J.|last3=Sana|first3=H.|last4=Walborn|first4=N. R.|last5=De Mink|first5=S. E.|author5-link=Selma de Mink|last6=Stroud|first6=V. E.|last7=Alvarez-Candal|first7=A.|last8=Barbá|first8=R. H.|last9=Bestenlehner|first9=J. M.|last10=Bonanos|first10=A. Z.|last11=Brott|first11=I.|year=2011|title=The VLT-FLAMES Tarantula Survey II: R139 revealed as a massive binary system|journal=Astronomy & Astrophysics|volume=530|pages=L10|arxiv=1103.5387|bibcode=2011A&A...530L..10T|doi=10.1051/0004-6361/201116785|first23=N.|first22=N.|last23=Morrell|first21=J.|last24=Monaco|first24=L.|last25=Vink|first25=J. S.|last22=Markova|first15=G.|last21=Maíz Apellániz|last16=Hénault-Brunet|last12=Crowther|first12=P. A.|last13=De Koter|first13=A.|last14=Friedrich|first14=K.|last15=Gräfener|first16=V.|first20=D. J.|last17=Herrero|first17=A.|last18=Kaper|first18=L.|last19=Langer|first19=N.|last20=Lennon|s2cid=119214376}}</ref><ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[VFTS 259]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1259000
| -10.51
|164000
|13.65
|37700
|{{SIMBAD link|VFTS+259|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[VFTS 1031]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1259000
| -10.51
|164000
|13.89
|48000
|{{SIMBAD link|VFTS+1031|SIMBAD}}
|<ref name="Doran2013" />
|-
| style="background: {{star-color|WC}};" |[[Sk -69° 194]] (位于[[大麦哲伦星系]]内的[[NGC 2033]])
|1247000
| -10.5
|160000
|12.131
|45000
|{{SIMBAD link|Sk+-69+194|SIMBAD}}
|<ref name=":42" /><ref name="Ulaczyk">{{Cite journal|last1=Ulaczyk|first1=K.|last2=Szymański|first2=M. K.|last3=Udalski|first3=A.|last4=Kubiak|first4=M.|last5=Pietrzyński|first5=G.|last6=Soszyński|first6=I.|last7=Wyrzykowski|first7=Ł.|last8=Poleski|first8=R.|last9=Gieren|first9=W.|last10=Walker|first10=A. R.|last11=Garcia-Varela|first11=A.|date=1 June 2013|title=Variable Stars from the OGLE-III Shallow Survey in the Large Magellanic Cloud|url=https://ui.adsabs.harvard.edu/abs/2013AcA....63..159U/abstract|journal=Acta Astronomica|volume=63|issue=2|pages=159–179|arxiv=1306.4802|bibcode=2013AcA....63..159U|issn=0001-5237|s2cid=119228254|access-date=2021-07-11|archive-date=2022-03-07|archive-url=https://web.archive.org/web/20220307220256/https://ui.adsabs.harvard.edu/abs/2013AcA....63..159U/abstract|dead-url=no}}</ref>
|-
| style="background: {{star-color|O}};" |[[ST2-22]] (位于[[大麦哲伦星系]]内的[[NGC 2044]])
|1247000
| -10.5
|160000
|14.3
|51300
|{{SIMBAD link|ST92+2-22|SIMBAD}}
|<ref name=":42" /><ref name="Schild" />
|-
| style="background: {{star-color|O}};" |[[川普勒27]]-27 (位于[[川普勒27]])
|1247000
| -10.5
|8200
|13.31
|37000
|{{SIMBAD link|Cl+Trumpler+27+27|SIMBAD}}
|<ref name="Massey et al. 2001" /><ref name="zacharias" />
|-
| style="background: {{star-color|O}};" |[[HSH95-47]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1230000
| -10.485
|163000
|14.72
|47000
|{{SIMBAD link|HSH95+47|SIMBAD}}
|<ref name="bestenlehner2020" /><ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[VFTS 1028]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1230000
| -10.485
|164000
|13.84
|47300
|{{SIMBAD link|VFTS+1028|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[LH 10]]-3601 (位于[[大麦哲伦星系]]内的[[NGC 1763]])
|1202000
| -10.46
|160000
|13.491
|55000
|{{SIMBAD link|L72+LH+10-3061|SIMBAD}}
|<ref name=":0" /><ref name=":7" />
|-
| style="background: {{star-color|WC}};" |[[AB1]] (位于[[小麦哲伦星系]]内的[[DEM S10]])
|1175000
| -10.435
|197000
|15.238
|79000
|{{SIMBAD link|SMC+AB+1|SIMBAD}}
|<ref name=":1">{{Cite journal|last1=Hainich|first1=R.|last2=Pasemann|first2=D.|last3=Todt|first3=H.|last4=Shenar|first4=T.|last5=Sander|first5=A.|last6=Hamann|first6=W. -R|date=2015|title=Wolf-Rayet stars in the Small Magellanic Cloud. I. Analysis of the single WN stars|journal=Astronomy & Astrophysics|volume=581|issue=21|page=30|arxiv=1507.04000|bibcode=2015A&A...581A..21H|doi=10.1051/0004-6361/201526241|s2cid=56230998}}</ref><ref name=":6" />
|-
| style="background: {{star-color|O}};" |[[BI 253]] (来自[[大麦哲伦星系]]内的[[蜘蛛星云]]的[[速逃星]])
|1175000
| -10.435
|164000
|13.76
|54000
|{{SIMBAD link|BI+253|SIMBAD}}
|<ref name="schneider2018" /><ref>{{Cite journal|last1=Rivero González|first1=J. G.|last2=Puls|first2=J.|last3=Najarro|first3=F.|last4=Brott|first4=I.|date=2012|title=Nitrogen line spectroscopy of O-stars. II. Surface nitrogen abundances for O-stars in the Large Magellanic Cloud|url=http://www.aanda.org/10.1051/0004-6361/201117790|journal=Astronomy & Astrophysics|volume=537|page=A79|arxiv=1110.5148|bibcode=2012A&A...537A..79R|doi=10.1051/0004-6361/201117790|issn=0004-6361|s2cid=119110554}}</ref>
|-
| style="background: {{star-color|O}};" |[[LGGS J013248.26+303950.4]] (位于[[三角座星系]])
|1175000
| -10.435
|3000000
|17.25
|23000
|{{SIMBAD link|LGGS+J013248.26%2B303950.4|SIMBAD}}
|<ref name=":2" /><ref>{{Cite journal|last1=Thompson|first1=Todd A.|last2=Prieto|first2=José L.|last3=Stanek|first3=K. Z.|last4=Kistler|first4=Matthew D.|last5=Beacom|first5=John F.|last6=Kochanek|first6=Christopher S.|date=2009-11-10|title=A New Class of Luminous Transients and a First Census of Their Massive Stellar Progenitors|url=https://iopscience.iop.org/article/10.1088/0004-637X/705/2/1364|journal=The Astrophysical Journal|volume=705|issue=2|pages=1364–1384|arxiv=0809.0510|bibcode=2009ApJ...705.1364T|doi=10.1088/0004-637X/705/2/1364|issn=0004-637X|hdl=1811/48176|s2cid=17581579}}</ref>
|-
| style="background: {{star-color|WC}};" |[[默瑟30]]-8 (位于[[龙鱼星云]]内的[[默瑟30]])
|1175000
| -10.435
|40000
|11.658 (J波段)
|38100
|{{SIMBAD link|DNB2016+Mc30-8|SIMBAD}}
|<ref name=":17" />
|-
| style="background: {{star-color|O}};" |[[NGC 346]]-W3 (位于[[小麦哲伦星系]]内的[[NGC 346]])
|1175000
| -10.435
|200000
|12.8
|52500
|{{SIMBAD link|Cl*+NGC+346+W+3|SIMBAD}}
|<ref name=":0" /><ref name=":6" />
|-
| style="background: {{star-color|WC}};" |[[五合星团|WR 102d]] (位于[[五合星团]])
|1175000
| -10.435
|26000
|15.18 (J波段)
|35100
|{{SIMBAD link|WR+102d|SIMBAD}}
|<ref name="quintuplet" /><ref name="qc" />
|-
| style="background: {{star-color|WC}};" |[[WR 126]] (位于[[狐狸座OB2]])
|1175000
| -10.435
|24680
|13.29
|63000
|{{SIMBAD link|WR+126|SIMBAD}}
|<ref name="sander2019">{{cite journal|last1=Sander|first1=A. A. C.|last2=Hamann|first2=W.-R.|last3=Todt|first3=H.|last4=Hainich|first4=R.|last5=Shenar|first5=T.|last6=Ramachandran|first6=V.|last7=Oskinova|first7=L. M.|year=2019|title=The Galactic WC and WO stars|journal=Astronomy & Astrophysics|volume=621|page=A92|arxiv=1807.04293|bibcode=2019A&A...621A..92S|doi=10.1051/0004-6361/201833712|s2cid=67754788}}</ref><ref name="zacharias" />
|-
| style="background: {{star-color|WC}};" |[[WR 20a]] A (位于[[维斯特卢2]])
|1150000
| -10.412
|20000
|13.28
|43000
|{{SIMBAD link|WR+20a|SIMBAD}}
|<ref name="Rauw2005">{{cite journal|author=Rauw|display-authors=etal|date=4 March 2005|title=The spectrum of the very massive binary system WR 20a (WN6ha + WN6ha): Fundamental parameters and wind interactions|url=https://pure.uva.nl/ws/files/2178609/46516_211088y.pdf|journal=Astronomy & Astrophysics|volume=432|issue=3|pages=985–998|bibcode=2005A&A...432..985R|doi=10.1051/0004-6361:20042136|doi-access=free|access-date=2021-07-11|archive-date=2020-08-03|archive-url=https://web.archive.org/web/20200803093658/https://pure.uva.nl/ws/files/2178609/46516_211088y.pdf|dead-url=no}}</ref>
|-
| style="background: {{star-color|WC}};" |[[WR 20a]] B (位于[[维斯特卢2]])
|1150000
| -10.412
|20000
|13.28
|43000
|{{SIMBAD link|WR+20a|SIMBAD}}
|<ref name="Rauw2005" />
|-
| style="background: {{star-color|WC}};" |[[GCIRS 16SW]] A (位于[[银心]])
|1149000
| -10.411
|26000
|15.5 (J波段)
|24400
|{{SIMBAD link|GCIRS+16SW|SIMBAD}}
|<ref name=":12">{{Cite journal|last1=Peeples|first1=Molly S.|last2=Bonanos|first2=A. Z.|last3=DePoy|first3=D. L.|last4=Stanek|first4=K. Z.|last5=Pepper|first5=J.|last6=Pogge|first6=Richard W.|last7=Pinsonneault|first7=M. H.|last8=Sellgren|first8=K.|date=2007-01-01|title=The Nature of the Variable Galactic Center Source GCIRS 16SW Revisited: A Massive Eclipsing Binary|url=https://iopscience.iop.org/article/10.1086/510720|journal=The Astrophysical Journal|volume=654|issue=1|pages=L61–L64|arxiv=astro-ph/0610212|bibcode=2007ApJ...654L..61P|doi=10.1086/510720|issn=0004-637X|s2cid=14242573|access-date=2021-07-11|archive-date=2021-01-21|archive-url=https://web.archive.org/web/20210121222831/https://iopscience.iop.org/article/10.1086/510720|dead-url=no}}</ref>
|-
| style="background: {{star-color|WC}};" |[[GCIRS 16SW]] B (位于[[银心]])
|1149000
| -10.411
|26000
|15.5 (J波段)
|23500
|{{SIMBAD link|GCIRS+16SW|SIMBAD}}
|<ref name=":12" />
|-
| style="background: {{star-color|WC}};" |[[BAT99-104]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1148000
| -10.41
|165000
|14.52
|63000
|{{SIMBAD link|BAT99+104|SIMBAD}}
|<ref name="hainich" /><ref name="Doran2013" />
|-
| style="background: {{star-color|WC}};" |[[CXOGC J174516.7-285824]] (位于[[银心]])
|1148000
| -10.41
|26000
|16.67 (J波段)
|35000
|{{SIMBAD link|CXOGC+J174516.7-285824|SIMBAD}}
|<ref name=":21" />
|-
| style="background: {{star-color|WC}};" |[[G0.121-0.099]] (位于[[银心]])
|1148000
| -10.41
|26000
|14.972 (J波段)
|40000
|{{SIMBAD link|MCD2010+G0.121-0.099|SIMBAD}}
|<ref name="mcd2010" />
|-
| style="background: {{star-color|B}};" |[[G359.797+0.037]] (位于[[银心]])
|1148000
| -10.41
|26000
|16.1 (J波段)
|30000
|{{SIMBAD link|MCD2010+G329.797%2B0.037|SIMBAD}}
|<ref name="mcd2010" />
|-
| style="background: {{star-color|O}};" |[[HD 93205]] A (位于[[船底座星云]]内的[[川普勒16]])
|1148000
| -10.41
|7500
|7.75
|51300
|{{SIMBAD link|HD+93205|SIMBAD}}
|<ref name="morrell">{{cite journal|last1=Morrell|first1=N. I.|author-link1=Nidia Morrell|last2=Barbá|first2=R. H.|last3=Niemela|first3=V. S.|last4=Corti|first4=M. A.|last5=Albacete Colombo|first5=J. F.|last6=Rauw|first6=G.|last7=Corcoran|first7=M.|last8=Morel|first8=T.|last9=Bertrand|first9=J.-F.|last10=Moffat|first10=A. F. J.|last11=St-Louis|first11=N.|year=2001|title=Optical spectroscopy of X-Mega targets - II. The massive double-lined O-type binary HD 93205|url=http://orbi.ulg.ac.be/bitstream/2268/34118/1/0105014.pdf|journal=Monthly Notices of the Royal Astronomical Society|volume=326|issue=1|pages=85–94|arxiv=astro-ph/0105014|bibcode=2001MNRAS.326...85M|doi=10.1046/j.1365-8711.2001.04500.x|s2cid=16221731|access-date=2021-07-11|archive-date=2017-08-18|archive-url=https://web.archive.org/web/20170818015925/http://orbi.ulg.ac.be/bitstream/2268/34118/1/0105014.pdf|dead-url=no}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|WC}};" |[[WR 158]] (位于[[仙后座OB1]])
|1148000
| -10.41
|16300
|11.282
|44700
|{{SIMBAD link|WR+158|SIMBAD}}
|<ref name="WN" /><ref name=":9" />
|-
| style="background: {{star-color|WC}};" |[[WR 28]] (位于[[FSR 1555]])
|1148000
| -10.41
|18700
|12.98
|50100
|{{SIMBAD link|WR+28|SIMBAD}}
|<ref name="WN" /><ref name="zacharias" />
|-
| style="background: {{star-color|O}};" |[[川普勒16|HD 303308]] (位于[[船底座星云]]内的[[川普勒16]])
|1138000
| -10.4
|7500
|8.17
|51300
|{{SIMBAD link|HD+303308|SIMBAD}}
|<ref name="Massey et al. 2001" /><ref name="ducati" />
|-
| style="background: {{star-color|WC}};" |[[M33C-15235]] (位于[[三角座星系]])
|1138000
| -10.4
|3000000
|17.73
|29200
|{{SIMBAD link|LGGS+J013351.46%2B304057.0|SIMBAD}}
|<ref name="humphreys2017" /><ref name=":10">{{Cite journal|last1=Neugent|first1=Kathryn F.|last2=Massey|first2=Philip|date=2011-06-01|title=The Wolf-Rayet Content of M33|url=https://iopscience.iop.org/article/10.1088/0004-637X/733/2/123|journal=The Astrophysical Journal|volume=733|issue=2|page=123|arxiv=1103.5549|bibcode=2011ApJ...733..123N|doi=10.1088/0004-637X/733/2/123|issn=0004-637X|s2cid=118507918|access-date=2021-07-11|archive-date=2021-06-06|archive-url=https://web.archive.org/web/20210606181745/https://iopscience.iop.org/article/10.1088/0004-637X/733/2/123|dead-url=no}}</ref>
|-
| style="background: {{star-color|WC}};" |[[AB9]] (位于[[小麦哲伦星系]]内的[[DEM S80]])
|1122000
| -10.385
|197000
|15.431
|100000
|{{SIMBAD link|SMC+AB+9|SIMBAD}}
|<ref name=":1" /><ref name=":6" />
|-
| style="background: {{star-color|O}};" |[[圆拱星团]]-F18 (位于[[圆拱星团]])
|1122000
| -10.385
|25000
|16.7 (J波段)
|36900
|{{SIMBAD link|FNG2002+18|SIMBAD}}
|<ref name="martins" /><ref name=":5" />
|-
| style="background: {{star-color|WC}};" |[[BAT99-64]] A (位于[[大麦哲伦星系]]内的[[NGC 2033]])
|1122000
| -10.385
|165000
|14.073
|71000
|{{SIMBAD link|BAT99+64|SIMBAD}}
|<ref name="hainich" /><ref name=":7" />
|-
| style="background: {{star-color|O}};" |[[HSH95-48]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1122000
| -10.385
|163000
|14.75
|49000
|{{SIMBAD link|HSH95+48|SIMBAD}}
|<ref name="bestenlehner2020" /><ref name="Doran2013" />
|-
| style="background: {{star-color|WN}};" |[[Var B]] (位于[[三角座星系]])
|1122000
| -10.385
|3000000
|16.208
|9000
|{{SIMBAD link|VHK+B|SIMBAD}}
|<ref name="Szeifert et al. 1996" /><ref name=":4" />
|-
| style="background: {{star-color|O}};" |[[VFTS 562]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1122000
| -10.385
|164000
|13.66
|42200
|{{SIMBAD link|VFTS+562|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
| style="background: {{star-color|WC}};" |[[WR 37]] (位于[[G291.27-0.71]]内的[[SFC 27]])
|1122000
| -10.385
|21900
|16
|100000
|{{SIMBAD link|WR+37|SIMBAD}}
|<ref name="WN" /><ref name="zacharias" />
|-
| style="background: {{star-color|O}};" |[[VFTS 512]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1096000
| -10.36
|164000
|14.28
|47700
|{{SIMBAD link|VFTS+512|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[默瑟30]]-6b (位于[[龙鱼星云]]内的[[默瑟30]])
|1072000
| -10.335
|40000
|14.25 (J波段)
|30500
|{{SIMBAD link|DNB2016+Mc30-6b|SIMBAD}}
|<ref name=":17" />
|-
| style="background: {{star-color|B}};" |[[VFTS 3]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1072000
| -10.335
|164000
|11.56
|21000
|{{SIMBAD link|VFTS+3|SIMBAD}}
|<ref name="schneider2018" /><ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[VFTS 151]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1072000
| -10.335
|164000
|14.13
|42200
|{{SIMBAD link|VFTS+151|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[VFTS 603]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1060000
| -10.323
|164000
|13.99
|43400
|{{SIMBAD link|VFTS+603|SIMBAD}}
|<ref>{{Cite journal|last1=Walborn|first1=N. R.|last2=Sana|first2=H.|last3=Simón-Díaz|first3=S.|last4=Maíz Apellániz|first4=J.|last5=Taylor|first5=W. D.|last6=Evans|first6=C. J.|last7=Markova|first7=N.|last8=Lennon|first8=D. J.|last9=de Koter|first9=A.|date=2014|title=The VLT-FLAMES Tarantula Survey. XIV. The O-type stellar content of 30 Doradus|journal=Astronomy & Astrophysics|volume=564|issue=40|page=35|arxiv=1402.6969|bibcode=2014A&A...564A..40W|doi=10.1051/0004-6361/201323082|s2cid=119302111}}</ref><ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[CXOGC J174532.7-285126]] (位于[[银心]])
|1047000
| -10.31
|26000
|10.72 (J波段)
|40000
|{{SIMBAD link|CXOGC+J174532.7-285126|SIMBAD}}
|<ref name=":21" />
|-
| style="background: {{star-color|O}};" |[[HD 93403]] A (位于[[船底座星云]]内的[[川普勒16]])
|1047000
| -10.31
|10000
|8.27
|39300
|{{SIMBAD link|HD+93403|SIMBAD}}
|<ref name="rauw">{{cite journal|last1=Rauw|first1=G.|last2=Vreux|first2=J.-M.|last3=Stevens|first3=I. R.|last4=Gosset|first4=E.|last5=Sana|first5=H.|last6=Jamar|first6=C.|last7=Mason|first7=K. O.|year=2002|title=Phase-resolved X-ray and optical spectroscopy of the massive binary HD 93403|journal=Astronomy and Astrophysics|volume=388|issue=2|page=552|bibcode=2002A&A...388..552R|doi=10.1051/0004-6361:20020523|doi-access=free}}</ref><ref name="zacharias" />
|-
| style="background: {{star-color|O}};" |[[默瑟30]]-2 (位于[[龙鱼星云]]内的[[默瑟30]])
|1047000
| -10.31
|40000
|12.63 (J波段)
|21200
|{{SIMBAD link|DNB2016+Mc30-2|SIMBAD}}
|<ref name=":17" />
|-
| style="background: {{star-color|O}};" |[[R133]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1047000
| -10.31
|163000
|12.49
|37600
|{{SIMBAD link|RMC133|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[HD 97950]] E (位于[[NGC 3603]]内的[[HD 97950]])
|1038000
| -10.3
|24000
|13.081
|46500
|{{SIMBAD link|HD+97950E|SIMBAD}}
|<ref name="melena2008" /><ref name=":16" />
|-
| style="background: {{star-color|B}};" |[[HD 229059]] (位于[[伯克利87]])
|1038000
| -10.3
|3200
|8.7
|26300
|{{SIMBAD link|HD+229059|SIMBAD}}
|<ref name="Massey et al. 2001" /><ref name="ducati" />
|-
| style="background: {{star-color|WC}};" |[[M33C-10788]] (位于[[三角座星系]])
|1038000
| -10.3
|3000000
|17.95
|32000
|{{SIMBAD link|LGGS+J013416.07%2B303642.1|SIMBAD}}
|<ref name="humphreys2017" /><ref name=":10" />
|-
| style="background: {{star-color|B}};" |[[Sk -69° 200]] (位于[[大麦哲伦星系]]内的[[NGC 2033]])
|1038000
| -10.3
|160000
|11.18
|26300
|{{SIMBAD link|Sk+-69+200|SIMBAD}}
|<ref name=":42" /><ref name="zacharias" />
|-
| style="background: {{star-color|B}};" |[[Sk -69° 259]] (位于[[大麦哲伦星系]]内的[[NGC 2081]])
|1038000
| -10.3
|160000
|11.93
|30000
|{{SIMBAD link|Sk+-69+259|SIMBAD}}
|<ref name=":42" /><ref name="zacharias" />
|-
| style="background: {{star-color|WC}};" |[[WR 77k]] (位于[[维斯特卢1]])
|1038000
| -10.3
|11000
|18.86
|35000
|{{SIMBAD link|WR+77k|SIMBAD}}
|<ref>{{Cite journal|last1=Crowther|first1=P. A.|last2=Hadfield|first2=L. J.|last3=Clark|first3=J. S.|last4=Negueruela|first4=I.|last5=Vacca|first5=W. D.|date=2006-11-01|title=A census of the Wolf-Rayet content in Westerlund 1 from near-infrared imaging and spectroscopy|url=https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2006.10952.x|journal=Monthly Notices of the Royal Astronomical Society|volume=372|issue=3|pages=1407–1424|arxiv=astro-ph/0608356|bibcode=2006MNRAS.372.1407C|doi=10.1111/j.1365-2966.2006.10952.x|issn=0035-8711|s2cid=10505573}}</ref><ref>{{Cite journal|last1=Clark|first1=J. S.|last2=Muno|first2=M. P.|last3=Negueruela|first3=I.|last4=Dougherty|first4=S. M.|last5=Crowther|first5=P. A.|last6=Goodwin|first6=S. P.|last7=de Grijs|first7=R.|date=2008|title=Unveiling the X-ray point source population of the Young Massive Cluster Westerlund 1|url=http://www.aanda.org/10.1051/0004-6361:20077186|journal=Astronomy & Astrophysics|volume=477|issue=1|pages=147–163|bibcode=2008A&A...477..147C|doi=10.1051/0004-6361:20077186|issn=0004-6361|doi-access=free}}</ref>
|-
| style="background: {{star-color|O}};" |[[HD 93250]] A (位于[[船底座星云]]内的[[川普勒16]])
|1023000
| -10.285
|7500
|7.5
|46000
|{{SIMBAD link|HD+93250|SIMBAD}}
|<ref name="repolust">{{cite journal|last1=Repolust|first1=T.|last2=Puls|first2=J.|last3=Herrero|first3=A.|year=2004|title=Stellar and wind parameters of Galactic O-stars. The influence of line-blocking/blanketing|journal=Astronomy and Astrophysics|volume=415|page=349|bibcode=2004A&A...415..349R|doi=10.1051/0004-6361:20034594|doi-access=free}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[HSH95-31]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1023000
| -10.285
|163000
|14.12
|48000
|{{SIMBAD link|HSH95+31|SIMBAD}}
|<ref name="bestenlehner2020" /><ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[VFTS 267]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1023000
| -10.285
|164000
|13.49
|44700
|{{SIMBAD link|VFTS+267|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[VFTS 599]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1023000
| -10.285
|164000
|13.8
|47300
|{{SIMBAD link|VFTS+599|SIMBAD}}
|<ref name="schneider2018" /><ref name="Doran2013" />
|-
| style="background: {{star-color|WC}};" |[[VVV CL074]]-9 (位于[[VVV CL074]])
|1023000
| -10.285
|20000
|15.22 (J波段)
|37000
|{{SIMBAD link|CBB2013+VVV+CL074+9|SIMBAD}}
|<ref name=":11" />
|-
| style="background: {{star-color|WC}};" |[[WR 156]] (位于[[仙王座OB1]])
|1023000
| -10.285
|13400
|11.01
|39800
|{{SIMBAD link|WR+156|SIMBAD}}
|<ref name="WN" /><ref name="tycho2" />
|-
| style="background: {{star-color|WC}};" |[[圆拱星团]]-F2 (WR 102aa 位于[[圆拱星团]])
|1000000
| -10.26
|25000
|17.84 (J波段)
|33500
|{{SIMBAD link|FNG2002+2|SIMBAD}}
|<ref name="martins" /><ref name=":5" />
|-
| style="background: {{star-color|WC}};" |[[圆拱星团]]-F14 (WR 102ba 位于[[圆拱星团]])
|1000000
| -10.26
|25000
|16.38 (J波段)
|34500
|{{SIMBAD link|FNG2002+14|SIMBAD}}
|<ref name="martins" /><ref name=":5" />
|-
| style="background: {{star-color|WC}};" |[[BAT99-68]] (位于[[大麦哲伦星系]]内的[[BSDL 2505]])
|1000000
| -10.26
|163000
|14.13
|45000
|{{SIMBAD link|BAT99+68|SIMBAD}}
|<ref name="hainich" /><ref>{{Cite journal|last1=Neugent|first1=Kathryn F.|last2=Massey|first2=Philip|last3=Morrell|first3=Nidia|date=2012-12-01|title=The Discovery of a Rare Wo-Type Wolf–Rayet Star in the Large Magellanic Cloud|url=https://iopscience.iop.org/article/10.1088/0004-6256/144/6/162|journal=The Astronomical Journal|volume=144|issue=6|page=162|arxiv=1210.0062|bibcode=2012AJ....144..162N|doi=10.1088/0004-6256/144/6/162|issn=0004-6256|s2cid=118628394|access-date=2021-07-11|archive-date=2021-10-26|archive-url=https://web.archive.org/web/20211026203918/https://iopscience.iop.org/article/10.1088/0004-6256/144/6/162|dead-url=no}}</ref>
|-
| style="background: {{star-color|O}};" |[[CXOGC J174628.2-283920]] (位于[[银心]])
|1000000
| -10.26
|26000
|16.99 (J波段)
|40000
|{{SIMBAD link|CXOGC+J174628.2-283920|SIMBAD}}
|<ref name=":21" />
|-
| style="background: {{star-color|O}};" |[[CXOGC J174703.1-283119]] (位于[[银心]])
|1000000
| -10.26
|26000
|16.23 (J波段)
|40000
|{{SIMBAD link|CXOGC+J174703.1-283119|SIMBAD}}
|<ref name=":21" />
|-
| style="background: {{star-color|O}};" |[[HSH95-28]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1000000
| -10.26
|163000
|14.09
|48000
|{{SIMBAD link|HSH95+28|SIMBAD}}
|<ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[HSH95-57]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1000000
| -10.26
|163000
|14.8
|47000
|{{SIMBAD link|HSH95+57|SIMBAD}}
|<ref name="Doran2013" />
|-
| style="background: {{star-color|WC}};" |[[R135]] A (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1000000
| -10.26
|163000
|13.48
|50000
|{{SIMBAD link|RMC135|SIMBAD}}
|<ref name="hainich" /><ref name="Doran2013" />
|-
| style="background: {{star-color|WC}};" |[[R140a2]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1000000
| -10.26
|163000
|12.12
|34000
|{{SIMBAD link|RMC140a2|SIMBAD}}
|<ref name="Doran2013" />
|-
| style="background: {{star-color|B}};" |[[R142]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1000000
| -10.26
|163000
|11.82
|21000
|{{SIMBAD link|RMC142|SIMBAD}}
|<ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[VFTS 64]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1000000
| -10.26
|164000
|14.62
|39800
|{{SIMBAD link|VFTS+64|SIMBAD}}
|<ref name="best" /><ref name="Doran2013" />
|-
| style="background: {{star-color|B}};" |[[VFTS 591]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1000000
| -10.26
|164000
|12.55
|27000
|{{SIMBAD link|VFTS+591|SIMBAD}}
|<ref name="Doran2013" />
|-
| style="background: {{star-color|O}};" |[[VFTS 1034]] (位于[[大麦哲伦星系]]内的[[蜘蛛星云]])
|1000000
| -10.26
|164000
|13.36
|34000
|{{SIMBAD link|VFTS+1034|SIMBAD}}
|<ref name="Doran2013" />
|-
| style="background: {{star-color|WC}};" |[[VVV CL074]]-3 (位于[[VVV CL074]])
|1000000
| -10.26
|20000
|14.72 (J波段)
|31500
|{{SIMBAD link|CBB2013+VVV+CL074+3|SIMBAD}}
|<ref name=":11" />
|}

'''一些常见的光度在1百万太阳光度之下的恒星：'''
{| class="wikitable sortable"
!恒星名称
![[輻射熱光度]](太陽=1)
![[絕對熱星等]]
!距離([[光年]])
![[视星等]]
![[有效温度]]([[开尔文|K]])
!链接
!參考文獻
|-
| style="background: {{star-color|B}};" |[[尾宿三]] (位于[[天蝎座OB1]]内的[[NGC 6231]])
|851000
| -10.085
|8210
| style="background: lightblue;" |4.705
|17200
|{{SIMBAD link|Zeta1+Scorpii|SIMBAD}}
|<ref name=":14">{{Cite journal|last1=Clark|first1=J. S.|last2=Najarro|first2=F.|last3=Negueruela|first3=I.|last4=Ritchie|first4=B. W.|last5=Urbaneja|first5=M. A.|last6=Howarth|first6=I. D.|date=2012|title=On the nature of the galactic early-B hypergiants|url=http://www.aanda.org/10.1051/0004-6361/201117472|journal=Astronomy & Astrophysics|volume=541|page=A145|arxiv=1202.3991|bibcode=2012A&A...541A.145C|doi=10.1051/0004-6361/201117472|issn=0004-6361|s2cid=11978733}}</ref><ref name="aass61_387">{{citation|last1=Kozok|first1=J. R.|title=Photometric observations of emission B-stars in the southern Milky Way|date=September 1985|journal=Astronomy and Astrophysics Supplement Series|volume=61|pages=387–405|bibcode=1985A&AS...61..387K}}</ref>
|-
| style="background: {{star-color|O}};" |[[弧矢增二十二]] (位于[[船帆座分子云脊]]内的[[船帆座R2]])
|813000
| -10.035
|1080
| style="background: lightblue;" |2.25
|40000
|{{SIMBAD link|Zeta+Puppis|SIMBAD}}
|<ref name="bouret2">{{cite journal|last1=Bouret|first1=J. -C.|last2=Hillier|first2=D. J.|last3=Lanz|first3=T.|last4=Fullerton|first4=A. W.|year=2012|title=Properties of Galactic early-type O-supergiants: A combined FUV-UV and optical analysis|journal=Astronomy & Astrophysics|volume=544|page=A67|arxiv=1205.3075v1|bibcode=2012A&A...544A..67B|doi=10.1051/0004-6361/201118594|s2cid=119280104}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[少卫 (右垣)|少卫/紫微右垣六]] (来自[[NGC 1502]]的[[速逃星]])
|676000
| -9.835
|6000
| style="background: lightblue;" |4.29
|29000
|{{SIMBAD link|Alpha+Camelopardalis|SIMBAD}}
|<ref name="repolust" /><ref name="ducati" />
|-
| style="background: {{star-color|WC}};" |[[天蝎座V919|WR 78]] (位于[[天蝎座OB1]]内的[[NGC 6231]])
|631000
| -9.76
|4100
| style="background: lightblue;" |6.48
|50100
|{{SIMBAD link|WR+78|SIMBAD}}
|<ref name="WN" /><ref name="gcvs" />
|-
| style="background: {{star-color|O}};" |[[造父三]] (来自[[仙王座OB3]]的[[速逃星]])
|631000
| -9.76
|3100
| style="background: lightblue;" |5.05
|36000
|{{SIMBAD link|Lambda+Cephei|SIMBAD}}
|<ref name="bouret2" /><ref name="ducati" />
|-
| style="background: {{star-color|WN}};" |[[天津增九]] (位于[[天鹅座OB1]]内的[[IC 4996]])
|610000
| -9.723
|5100
| style="background: lightblue;" |4.82
|18700
|{{SIMBAD link|P+Cygni|SIMBAD}}
|<ref name="rivet">{{cite journal|last1=Rivet|first1=J-P|last2=Siciak|first2=A.|last3=de Almeida|first3=E. S. G.|last4=Vakili|first4=F.|last5=Domiciano de Souza|first5=A.|last6=Fouché|first6=M.|last7=Lai|first7=O.|last8=Vernet|first8=D.|last9=Kaiser|first9=R.|last10=Guerin|first10=W.|year=2020|title=Intensity interferometry of P Cygni in the H α emission line: Towards distance calibration of LBV supergiant stars|journal=Monthly Notices of the Royal Astronomical Society|volume=494|pages=218–227|arxiv=1910.08366|bibcode=2020MNRAS.494..218R|doi=10.1093/mnras/staa588|s2cid=204788654}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|WC}};" |[[HD 152408|WR 79a]] (位于[[天蝎座OB1]]内的[[NGC 6231]])
|603000
| -9.71
|5600
| style="background: lightblue;" |5.77
|35000
|{{SIMBAD link|WR+79a|SIMBAD}}
|<ref>{{Cite journal|last1=Skinner|first1=Stephen L.|last2=Zhekov|first2=Svetozar A.|last3=Güdel|first3=Manuel|last4=Schmutz|first4=Werner|last5=Sokal|first5=Kimberly R.|date=2012-05-01|title=New X-Ray Detections of WNL Stars|url=https://iopscience.iop.org/article/10.1088/0004-6256/143/5/116|journal=The Astronomical Journal|volume=143|issue=5|page=116|arxiv=1203.5098|bibcode=2012AJ....143..116S|doi=10.1088/0004-6256/143/5/116|issn=0004-6256|s2cid=119281411|access-date=2021-07-11|archive-date=2021-06-05|archive-url=https://web.archive.org/web/20210605183531/https://iopscience.iop.org/article/10.1088/0004-6256/143/5/116|dead-url=no}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|B}};" |[[参宿二]] (位于[[猎户座分子云团]]内的[[猎户座OB1]])
|537000
| -9.585
|2000
| style="background: lightblue;" |1.69
|27500
|{{SIMBAD link|Epsilon+Orionis|SIMBAD}}
|<ref name="Searle 20082">{{cite journal|author=Searle, S. C.|author2=Prinja, R. K.|author3=Massa, D.|author4=Ryans, R.|date=2008|title=Quantitative studies of the optical and UV spectra of Galactic early B supergiants. I. Fundamental parameters|journal=Astronomy and Astrophysics|volume=481|issue=3|pages=777–97|arxiv=0801.4289|bibcode=2008A&A...481..777S|doi=10.1051/0004-6361:20077125|s2cid=1552752}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[海山二]] B (位于[[船底座星云]]内的[[川普勒16]])
|400000
| -9.265
|7500
| style="background: lightblue;" |4.3
|37200
|{{SIMBAD link|Eta+Carinae|SIMBAD}}
|<ref name="mehner">{{cite journal|last1=Mehner|first1=Andrea|last2=Davidson|first2=Kris|last3=Ferland|first3=Gary J.|last4=Humphreys|first4=Roberta M.|year=2010|title=High-excitation Emission Lines near Eta Carinae, and Its Likely Companion Star|journal=The Astrophysical Journal|volume=710|issue=1|pages=729–742|arxiv=0912.1067|bibcode=2010ApJ...710..729M|doi=10.1088/0004-637X/710/1/729|s2cid=5032987}}</ref><ref name="2018-07-02_NAL" />
|-
| style="background: {{star-color|B}};" |[[王良二]] (位于[[仙后座OB14]])
|302000
| -8.96
|4000
| style="background: lightblue;" |4.16
|23500
|{{SIMBAD link|Kappa+Cassiopeiae|SIMBAD}}
|<ref name="Searle 20082" /><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[弧矢增六]] Aa (位于[[NGC 2362]])
|299000
| -8.95
|5120
| style="background: lightblue;" |4.89
|32000
|{{SIMBAD link|Tau+Canis+Majoris|SIMBAD}}
|<ref name="an331_4_3492">{{citation|last1=Hohle|first1=M. M.|title=Masses and luminosities of O- and B-type stars and red supergiants|date=April 2010|journal=Astronomische Nachrichten|volume=331|issue=4|page=349|arxiv=1003.2335|bibcode=2010AN....331..349H|doi=10.1002/asna.200911355|last2=Neuhäuser|first2=R.|last3=Schutz|first3=B. F.|s2cid=111387483}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[天社一]] B (位于[[船帆座OB2]])
|280000
| -8.878
|1230
| style="background: lightblue;" |1.83
|35000
|{{SIMBAD link|Gamma2+Velorum|SIMBAD}}
|<ref name=":13" /><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[卷舌三]] (位于[[英仙座OB2]]内的[[加州星雲]])
|263000
| -8.81
|1200
| style="background: lightblue;" |4.04
|35000
|{{SIMBAD link|Xi+Persei|SIMBAD}}
|<ref name="repolust" /><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[参宿一]] Aa (位于[[猎户座分子云团]]内的[[猎户座OB1]])
|250000
| -8.755
|1260
| style="background: lightblue;" |2.08
|29500
|{{SIMBAD link|Zeta+Orionis|SIMBAD}}
|<ref>{{Cite journal|last1=Hummel|first1=C. A.|last2=Rivinius|first2=Th.|last3=Nieva|first3=M.-F.|last4=Stahl|first4=O.|last5=van Belle|first5=G.|last6=Zavala|first6=R. T.|date=2013|title=Dynamical mass of the O-type supergiant in ζ Orionis A|url=http://www.aanda.org/10.1051/0004-6361/201321434|journal=Astronomy & Astrophysics|volume=554|page=A52|arxiv=1306.0330|bibcode=2013A&A...554A..52H|doi=10.1051/0004-6361/201321434|issn=0004-6361|s2cid=53645495}}</ref>
|-
| style="background: {{star-color|WC}};" |[[苍蝇座θ]] Aa (位于[[半人马座OB1]])
|234000
| -8.685
|7400
| style="background: lightblue;" |5.53
|83000
|{{SIMBAD link|Theta+Muscae+A|SIMBAD}}
|<ref name="nugis">{{cite journal|last1=Nugis|first1=T.|last2=Lamers|first2=H. J. G. L. M.|year=2000|title=Mass-loss rates of Wolf-Rayet stars as a function of stellar parameters|journal=Astronomy and Astrophysics|volume=360|page=227|bibcode=2000A&A...360..227N}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|B}};" |[[大犬座ο²|军市增五]] (位于[[科林德121]])
|219000
| -8.61
|2800
| style="background: lightblue;" |3.043
|15500
|{{SIMBAD link|Omicron2+Canis+Majoris|SIMBAD}}
|<ref name="aaa446_1_279">{{citation|last1=Crowther|first1=P. A.|title=Physical parameters and wind properties of galactic early B supergiants|date=January 2006|journal=Astronomy and Astrophysics|volume=446|issue=1|pages=279–293|arxiv=astro-ph/0509436|bibcode=2006A&A...446..279C|doi=10.1051/0004-6361:20053685|last2=Lennon|first2=D. J.|last3=Walborn|first3=N. R.|s2cid=18815761}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[獵戶座θ1C|伐一C1]] (位于[[猎户座分子云团]]内的[[猎户四边形星团]])
|204000
| -8.535
|1340
| style="background: lightblue;" |5.13
|39000
|{{SIMBAD link|Theta1+Orionis+C|SIMBAD}}
|<ref>{{Cite journal|last1=Simón-Díaz|first1=S.|last2=Herrero|first2=A.|last3=Esteban|first3=C.|last4=Najarro|first4=F.|date=2006|title=Detailed spectroscopic analysis of the Trapezium cluster stars inside the Orion nebula: Rotational velocities, stellar parameters, and oxygen abundances|url=http://www.aanda.org/10.1051/0004-6361:20053066|journal=Astronomy & Astrophysics|volume=448|issue=1|pages=351–366|arxiv=astro-ph/0510288|bibcode=2006A&A...448..351S|doi=10.1051/0004-6361:20053066|issn=0004-6361|s2cid=16445304}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[参宿三]] Aa1 (位于[[猎户座分子云团]]内的[[猎户座OB1]])
|191000
| -8.46
|1200
| style="background: lightblue;" |2.5
|29500
|{{SIMBAD link|Delta+Orionis+A|SIMBAD}}
|<ref name="shenar2015">{{cite journal|last1=Shenar|first1=T.|last2=Oskinova|first2=L.|last3=Hamann|first3=W.-R.|last4=Corcoran|first4=M. F.|last5=Moffat|first5=A. F. J.|last6=Pablo|first6=H.|last7=Richardson|first7=N. D.|last8=Waldron|first8=W. L.|last9=Huenemoerder|first9=D. P.|last10=Maíz Apellániz|first10=J.|last11=Nichols|first11=J. S.|year=2015|title=A Coordinated X-Ray and Optical Campaign of the Nearest Massive Eclipsing Binary, δ Orionis Aa. IV. A Multiwavelength, Non-LTE Spectroscopic Analysis|journal=Astrophysical Journal|volume=809|issue=2|page=135|arxiv=1503.03476|bibcode=2015ApJ...809..135S|doi=10.1088/0004-637X/809/2/135|first13=Y.|last16=Negueruela|last12=Todt|first12=H.|first16=I.|last13=Nazé|hdl=10045/59172|last15=Pollock|first14=J. L.|last14=Hoffman|first15=A. M. T.|s2cid=14909574}}</ref><ref name="tokovinin1997">{{cite journal|last1=Tokovinin|first1=A. A.|year=1997|title=MSC - a catalogue of physical multiple stars|journal=Astronomy and Astrophysics Supplement Series|volume=124|pages=75–84|bibcode=1997A&AS..124...75T|doi=10.1051/aas:1997181|doi-access=free}}</ref>
|-
| style="background: {{star-color|WC}};" |[[天社一]] A (位于[[船帆座OB2]])
|170000
| -8.336
|1230
| style="background: lightblue;" |1.83
|57000
|{{SIMBAD link|Gamma2+Velorum|SIMBAD}}
|<ref name=":13">{{Cite journal|last1=North|first1=J. R.|last2=Tuthill|first2=P. G.|last3=Tango|first3=W. J.|last4=Davis|first4=J.|date=2007-05-01|title=γ2 Velorum: orbital solution and fundamental parameter determination with SUSI|url=https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2007.11608.x|journal=Monthly Notices of the Royal Astronomical Society|volume=377|issue=1|pages=415–424|arxiv=astro-ph/0702375|bibcode=2007MNRAS.377..415N|doi=10.1111/j.1365-2966.2007.11608.x|issn=0035-8711|s2cid=16425744|access-date=2021-07-11|archive-date=2022-02-02|archive-url=https://web.archive.org/web/20220202172914/https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2007.11608.x|dead-url=no}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|B}};" |[[弧矢二]] (位于[[科林德121]])
|151000
| -8.21
|2000
| style="background: lightblue;" |2.45
|15000
|{{SIMBAD link|Eta+Canis+Majoris|SIMBAD}}
|<ref name="Searle 20082" /><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[觜宿一]] A (位于[[猎户座分子云团]]内的[[科林德69|猎户座λ星协]])
|150000
| -8.2
|1100
| style="background: lightblue;" |3.54
|37700
|{{SIMBAD link|Lambda+Orionis+A|SIMBAD}}
|<ref>{{Cite journal|last1=Murdin|first1=P.|last2=Penston|first2=M. V.|date=1977-12-01|title=The Lambda Orionis association|url=https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/181.4.657|journal=Monthly Notices of the Royal Astronomical Society|volume=181|issue=4|pages=657–665|bibcode=1977MNRAS.181..657M|doi=10.1093/mnras/181.4.657|issn=0035-8711|doi-access=free|access-date=2021-07-11|archive-date=2021-10-29|archive-url=https://web.archive.org/web/20211029010614/https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/181.4.657|dead-url=no}}</ref><ref name="hr">{{cite book|last1=Hoffleit|first1=Dorrit|title=The Bright star catalogue|last2=Jaschek|first2=Carlos|publisher=Yale University Observatory|year=1991|edition=5th Revised|location=New Haven, Conn.|bibcode=1991bsc..book.....H}}</ref>
|-
| style="background: {{star-color|B}};" |[[参宿七]] A (位于[[猎户座分子云团]]内的[[猎户座OB1]])
|120000
| -7.96
|860
| style="background: lightblue;" |0.13
|12100
|{{SIMBAD link|Beta+Orionis+A|SIMBAD}}
|<ref>{{Cite journal|last1=Moravveji|first1=Ehsan|last2=Guinan|first2=Edward F.|last3=Shultz|first3=Matt|last4=Williamson|first4=Michael H.|last5=Moya|first5=Andres|date=2012-03-10|title=Asteroseismology of the Nearby SN-II Progenitor: Rigel. I. Themosthigh-Precision Photometry and Radial Velocity Monitoring|url=https://iopscience.iop.org/article/10.1088/0004-637X/747/2/108|journal=The Astrophysical Journal|volume=747|issue=2|page=108|arxiv=1201.0843|bibcode=2012ApJ...747..108M|doi=10.1088/0004-637X/747/2/108|issn=0004-637X|s2cid=425831|access-date=2021-07-11|archive-date=2021-03-24|archive-url=https://web.archive.org/web/20210324004601/https://hkvalidate.perfdrive.com/?ssa=2deed19d-aa53-454b-b442-8a5b0e2ffffa&ssb=47994249832&ssc=https%3A%2F%2Fiopscience.iop.org%2Farticle%2F10.1088%2F0004-637X%2F747%2F2%2F108&ssi=094ebacd-8427-49bf-95e2-6c76ca14dace&ssk=support%40shieldsquare.com&ssm=12974105477895199108733256840866&ssn=e745b9968c2f70ad65872350a5e9fcd5b1d9f47e82dc-fb2f-4a4d-883aa1&sso=3275d1e6-6bf3c3def91b5796f45028c97f33599dcccb9ff5d015562a&ssp=39961890771616513777161651685906671&ssq=76951094676128369171646761669664898175388&ssr=MjA3LjI0MS4yMzIuMTg1&sst=Mozilla%2F5.0%20%28Windows%20NT%2010.0%3B%20Win64%3B%20x64%29%20AppleWebKit%2F537.36%20%28KHTML%2C%20like%20Gecko%29%20Chrome%2F74.0.3729.169%20Safari%2F537.36&ssv=&ssw=|dead-url=no}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[伐二]] A (位于[[猎户座分子云团]]内的[[猎户座OB1]])
|107000
| -7.833
|1500
| style="background: lightblue;" |5.02
|34900
|{{SIMBAD link|Theta2+Orionis+A|SIMBAD}}
|<ref name="hillendrand">{{cite journal|last1=Hillenbrand|first1=Lynne A.|year=1997|title=On the Stellar Population and Star-Forming History of the Orion Nebula Cluster|url=https://archive.org/details/sim_astronomical-journal_1997-05_113_1697/page/1733|journal=Astronomical Journal|volume=113|page=1733|bibcode=1997AJ....113.1733H|doi=10.1086/118389}}</ref><ref>{{cite journal|last1=Aldoretta|first1=E. J.|last2=Caballero-Nieves|first2=S. M.|last3=Gies|first3=D. R.|last4=Nelan|first4=E. P.|last5=Wallace|first5=D. J.|last6=Hartkopf|first6=W. I.|last7=Henry|first7=T. J.|last8=Jao|first8=W.-C.|last9=Maíz Apellániz|first9=J.|last10=Mason|first10=B. D.|last11=Moffat|first11=A. F. J.|year=2015|title=The Multiplicity of Massive Stars: A High Angular Resolution Survey with the Guidance Sensor|journal=The Astronomical Journal|volume=149|issue=1|page=26|arxiv=1410.0021|bibcode=2015AJ....149...26A|doi=10.1088/0004-6256/149/1/26|first13=N. D.|last14=Williams|first14=S. J.|last13=Richardson|first12=R. P.|last12=Norris|s2cid=58911264}}</ref>
|-
| style="background: {{star-color|O}};" |[[天市右垣十一]]/[[天市右垣十一|韩]] (位于[[天蝎-半人马星协]]内的[[天蝎-半人马星协|上天蝎次集团]])
|74100
| -7.435
|370
| style="background: lightblue;" |2.569
|34000
|{{SIMBAD link|Zeta+Ophiuchi|SIMBAD}}
|<ref name="repolust" /><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[伐三]] Aa1 (位于[[猎户座分子云团]]内的[[NGC 1980]])
|68000
| -7.341
|1340
| style="background: lightblue;" |2.77
|32500
|{{SIMBAD link|Iota+Orionis|SIMBAD}}
|<ref name="marchenko">{{cite journal|last1=Marchenko|first1=Sergey V.|last2=Rauw|first2=Gregor|last3=Antokhina|first3=Eleonora A.|last4=Antokhin|first4=Igor I.|last5=Ballereau|first5=Dominique|last6=Chauville|first6=Jacques|last7=Corcoran|first7=Michael F.|last8=Costero|first8=Rafael|last9=Echevarria|first9=Juan|last10=Eversberg|first10=Thomas|last11=Gayley|first11=Ken G.|year=2000|title=Coordinated monitoring of the eccentric O-star binary Iota Orionis: Optical spectroscopy and photometry|journal=Monthly Notices of the Royal Astronomical Society|volume=317|issue=2|page=333|bibcode=2000MNRAS.317..333M|doi=10.1046/j.1365-8711.2000.03542.x|doi-access=free|first12=Gloria|last18=Pittard|last12=Koenigsberger|first21=Jean|last21=Zorec|first20=Jean-Marie|last20=Vreux|first19=Ian R.|last19=Stevens|first16=Nancy D.|author12-link=Gloria Suzanne Koenigsberger Horowitz|first18=Julian M.|last16=Morrison|first15=Nidia I.|last15=Morrell|first14=Anthony F. J.|last14=Moffat|first13=Anatoly S.|last13=Miroshnichenko|last17=Mulliss|first17=Christopher L.}}</ref><ref name="aass34_1" />
|-
| style="background: {{star-color|O}};" |[[参宿增三十六]] (位于[[猎户座分子云团]]内的[[猎户座OB1]])
|60000
| -7.205
|2900
| style="background: lightblue;" |4.618
|33400
|{{SIMBAD link|Upsilon+Orionis|SIMBAD}}
|<ref name="underhill79">{{cite journal|author=Underhill, A. B.|author2=Divan, L.|author3=Prevot-Burnichon, M.-L.|author4=Doazan, V.|date=1979|title=Effective temperatures, angular diameters, distances and linear radii for 160 O and B stars|journal=[[Monthly Notices of the Royal Astronomical Society]]|volume=189|issue=3|pages=601–05|bibcode=1979MNRAS.189..601U|doi=10.1093/mnras/189.3.601|doi-access=free}}</ref><ref>{{Cite journal|last=Nieva|first=M.-F.|date=2013|title=Temperature, gravity, and bolometric correction scales for non-supergiant OB stars|url=http://www.aanda.org/10.1051/0004-6361/201219677|journal=Astronomy & Astrophysics|volume=550|page=A26|arxiv=1212.0928|bibcode=2013A&A...550A..26N|doi=10.1051/0004-6361/201219677|issn=0004-6361|s2cid=119275940}}</ref>
|-
| style="background: {{star-color|B}};" |[[参宿六]] (位于[[猎户座分子云团]]内的[[猎户座OB1]])
|57000
| -7.147
|650
| style="background: lightblue;" |2.09
|26500
|{{SIMBAD link|Kappa+Orionis|SIMBAD}}
|<ref name="an331_4_3492" /><ref name="ducati" />
|-
| style="background: {{star-color|B}};" |[[天津增二十八]] (位于[[天鹅座OB4]])
|52000
| -7.06
|3260
| style="background: lightblue;" |4.233
|10800
|{{SIMBAD link|Sigma+Cygni|SIMBAD}}
|<ref name="tanriverdi">{{cite journal|last1=Tanrıverdi|first1=Taner|year=2013|title=Elemental abundances of the supergiant stars σ Cygnus and η Leonis|journal=New Astronomy|volume=25|page=50|arxiv=1512.04557|bibcode=2013NewA...25...50T|doi=10.1016/j.newast.2013.03.013|s2cid=118525375}}</ref><ref name="firnstein">{{cite journal|last1=Firnstein|first1=M.|last2=Przybilla|first2=N.|year=2012|title=Quantitative spectroscopy of Galactic BA-type supergiants. I. Atmospheric parameters|journal=Astronomy & Astrophysics|volume=543|page=A80|arxiv=1207.0308|bibcode=2012A&A...543A..80F|doi=10.1051/0004-6361/201219034|s2cid=54725386}}</ref>
|-
| style="background: {{star-color|B}};" |[[卷舌四]] (位于[[英仙座OB2]])
|47000
| -6.941
|750
| style="background: lightblue;" |2.86
|20800
|{{SIMBAD link|Zeta+Persei|SIMBAD}}
|<ref name="an331_4_3492" /><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[天鸽座μ|屎]] (来自[[猎户四边形星团]]的[[速逃星]])
|46000
| -6.91
|1300
| style="background: lightblue;" |5.18
|33000
|{{SIMBAD link|mu+Columbae|SIMBAD}}
|<ref name=":15">{{Cite journal|last1=Martins|first1=F.|last2=Schaerer|first2=D.|last3=Hillier|first3=D. J.|last4=Meynadier|first4=F.|last5=Heydari-Malayeri|first5=M.|last6=Walborn|first6=N. R.|date=2005|title=O stars with weak winds: the Galactic case|url=http://www.aanda.org/10.1051/0004-6361:20052927|journal=Astronomy & Astrophysics|volume=441|issue=2|pages=735–762|arxiv=astro-ph/0507278|bibcode=2005A&A...441..735M|doi=10.1051/0004-6361:20052927|issn=0004-6361|s2cid=11547293}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|O}};" |[[参宿增一]] Aa (位于[[猎户座分子云团]]内的[[猎户座OB1]])
|41700
| -6.81
|1260
| style="background: lightblue;" |4.07
|35000
|{{SIMBAD link|Sigma+Orionis+A|SIMBAD}}
|<ref name="simondiaz2015">{{cite journal|last1=Simón-Díaz|first1=S.|last2=Caballero|first2=J. A.|last3=Lorenzo|first3=J.|last4=Maíz Apellániz|first4=J.|last5=Schneider|first5=F. R. N.|last6=Negueruela|first6=I.|last7=Barbá|first7=R. H.|last8=Dorda|first8=R.|last9=Marco|first9=A.|last10=Montes|first10=D.|last11=Pellerin|first11=A.|year=2015|title=Orbital and Physical Properties of the σ Ori Aa, Ab, B Triple System|journal=The Astrophysical Journal|volume=799|issue=2|page=169|arxiv=1412.3469|bibcode=2015ApJ...799..169S|doi=10.1088/0004-637X/799/2/169|first12=J.|last13=Sódor|first13=Á.|last14=Sota|first14=A.|last12=Sanchez-Bermudez|s2cid=118500350}}</ref><ref name="wds">{{cite journal|last1=Mason|first1=Brian D.|last2=Wycoff|first2=Gary L.|last3=Hartkopf|first3=William I.|last4=Douglass|first4=Geoffrey G.|last5=Worley|first5=Charles E.|year=2001|title=The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog|url=https://archive.org/details/sim_astronomical-journal_2001-12_122_6/page/3466|journal=The Astronomical Journal|volume=122|issue=6|page=3466|bibcode=2001AJ....122.3466M|doi=10.1086/323920|doi-access=free}}</ref>
|-
| style="background: {{star-color|B}};" |[[房宿三]] A (位于[[天蝎-半人马星协]]内的[[天蝎-半人马星协|上天蝎次集团]])
|38000
| -6.71
|440
| style="background: lightblue;" |2.307
|27400
|{{SIMBAD link|Delta+Scorpii|SIMBAD}}
|<ref name="Pecaut">{{Cite journal|last1=Pecaut|first1=Mark J.|last2=Mamajek|first2=Eric E.|last3=Bubar|first3=Eric J.|date=2012-02-20|title=A Revised Age for Upper Scorpius and the Star Formation History Among the F-Type Members of the Scorpius-Centaurus Ob Association|url=https://iopscience.iop.org/article/10.1088/0004-637X/746/2/154|journal=The Astrophysical Journal|volume=746|issue=2|page=154|arxiv=1112.1695|bibcode=2012ApJ...746..154P|doi=10.1088/0004-637X/746/2/154|issn=0004-637X|s2cid=118461108|access-date=2021-07-11|archive-date=2021-02-25|archive-url=https://web.archive.org/web/20210225094756/https://iopscience.iop.org/article/10.1088/0004-637X/746/2/154|dead-url=no}}</ref><ref>{{Cite journal|last1=Gutierrez-Moreno|first1=Adelina|last2=Moreno|first2=Hugo|date=1968-06-01|title=A Photometric Investigation of the SCORPlO-CENTAURUS Association|url=http://adsabs.harvard.edu/abs/1968ApJS...15..459G|journal=The Astrophysical Journal Supplement Series|volume=15|page=459|bibcode=1968ApJS...15..459G|doi=10.1086/190168|issn=0067-0049|access-date=2021-07-11|archive-date=2019-03-25|archive-url=https://web.archive.org/web/20190325085216/http://adsabs.harvard.edu/abs/1968ApJS...15..459G|dead-url=no}}</ref>
|-
| style="background: {{star-color|B}};" |[[卷舌二]] A (位于[[英仙座α星团]])
|28300
| -6.391
|640
| style="background: lightblue;" |2.88
|26500
|{{SIMBAD link|Epsilon+Persei|SIMBAD}}
|<ref name="an331_4_3492" /><ref name="aj82_431">{{citation|last1=Lutz|first1=T. E.|title=Spectral classification and UBV photometry of bright visual double stars|date=June 1977|journal=Astronomical Journal|volume=82|pages=431–434|bibcode=1977AJ.....82..431L|doi=10.1086/112066|last2=Lutz|first2=J. H.|author2-link=Julie Lutz}}</ref>
|-
| style="background: {{star-color|B}};" |[[南船三]] A (位于[[天蝎-半人马星协]]内的[[IC 2602]])
|25700
| -6.284
|460
| style="background: lightblue;" |2.76
|31000
|{{SIMBAD link|Theta+Carinae|SIMBAD}}
|<ref name="an331_4_3492" /><ref name="clpl4">{{citation|last1=Johnson|first1=H. L.|title=UBVRIJKL photometry of the bright stars|journal=Communications of the Lunar and Planetary Laboratory|volume=4|issue=99|page=99|year=1966|bibcode=1966CoLPL...4...99J|display-authors=1|last2=Iriarte|first2=B.|last3=Mitchell|first3=R. I.|last4=Wisniewskj|first4=W. Z.}}</ref>
|-
| style="background: {{star-color|B}};" |[[军市一]] (位于[[本地泡]])
|25000
| -6.26
|490
| style="background: lightblue;" |1.985
|23200
|{{SIMBAD link|Beta+Canis+Majoris|SIMBAD}}
|<ref name="mnras369_1_L61">{{citation|last1=Hubrig|first1=S.|title=Discovery of magnetic fields in the βCephei star ξ1 CMa and in several slowly pulsating B stars*|date=June 2006|journal=[[Monthly Notices of the Royal Astronomical Society: Letters]]|volume=369|issue=1|pages=L61–L65|arxiv=astro-ph/0604283|bibcode=2006MNRAS.369L..61H|doi=10.1111/j.1745-3933.2006.00175.x|display-authors=1|last2=Briquet|first2=M.|last3=Schöller|first3=M.|last4=De Cat|first4=P.|last5=Mathys|first5=G.|last6=Aerts|first6=C.|s2cid=18201908}}</ref><ref name="mnassa31_69">{{citation|last1=Cousins|first1=A. W. J.|title=UBV Photometry of Some Very Bright Stars|date=1972|journal=Monthly Notes of the Astronomical Society of Southern Africa|volume=31|page=69|bibcode=1972MNSSA..31...69C}}</ref>
|-
| style="background: {{star-color|O}};" |[[参宿增一]] Ab (位于[[猎户座分子云团]]内的[[猎户座OB1]])
|18600
| -5.934
|1260
| style="background: lightblue;" |4.07
|29000
|{{SIMBAD link|Sigma+Orionis+A|SIMBAD}}
|<ref name="simondiaz2015" /><ref name="wds" />
|-
| style="background: {{star-color|B}};" |[[参宿增一]] B (位于[[猎户座分子云团]]内的[[猎户座OB1]])
|15800
| -5.757
|1260
| style="background: lightblue;" |4.07
|31000
|{{SIMBAD link|Sigma+Orionis+B|SIMBAD}}
|<ref name="simondiaz2015" /><ref name="wds" />
|-
| style="background: {{star-color|B}};" |[[伐二]] B (位于[[猎户座分子云团]]内的[[猎户座OB1]])
|12300
| -5.485
|1500
| style="background: lightblue;" |6.38
|29300
|{{SIMBAD link|Theta2+Orionis+B|SIMBAD}}
|<ref name="nieva">{{cite journal|last1=Nieva|first1=María-Fernanda|last2=Przybilla|first2=Norbert|year=2014|title=Fundamental properties of nearby single early B-type stars|journal=Astronomy & Astrophysics|volume=566|page=A7|arxiv=1412.1418|bibcode=2014A&A...566A...7N|doi=10.1051/0004-6361/201423373|s2cid=119227033}}</ref>
|-
| style="background: {{star-color|B}};" |[[伐三]] Aa2 (位于[[猎户座分子云团]]内的[[NGC 1980]])
|8630
| -5.1
|1340
| style="background: lightblue;" |2.77
|27000
|{{SIMBAD link|Iota+Orionis|SIMBAD}}
|<ref name="marchenko" /><ref name="aass34_1" />
|-
| style="background: {{star-color|B}};" |[[毕宿八]] A (位于[[双鱼-波江座星流]])
|5800
| -4.669
|480
| style="background: lightblue;" |3.47
|18700
|{{SIMBAD link|Lambda+Tauri|SIMBAD}}
|<ref name="an331_4_3492" /><ref name="aaass34_1">{{cite journal|last1=Nicolet|first1=B.|date=October 1978|title=Catalogue of homogeneous data in the UBV photoelectric photometric system|journal=Astronomy and Astrophysics Supplement Series|volume=34|pages=1–49|bibcode=1978A&AS...34....1N}}</ref>
|-
| style="background: {{star-color|B}};" |[[心宿增四]] A (位于[[蛇夫座ρ星云复合体]])
|4000
| -4.285
|360
| style="background: lightblue;" |4.63
|22000
|{{SIMBAD link|Rho+Ophiuchi+A|SIMBAD}}
|<ref>{{Cite journal|last1=Pillitteri|first1=I.|last2=Fossati|first2=L.|last3=Castro Rodriguez|first3=N.|last4=Oskinova|first4=L.|last5=Wolk|first5=S. J.|date=2018|title=Detection of magnetic field in the B2 star ρ Ophiuchi A with ESO FORS2|url=https://www.aanda.org/10.1051/0004-6361/201732078|journal=Astronomy & Astrophysics|volume=610|page=L3|arxiv=1712.00728|bibcode=2018A&A...610L...3P|doi=10.1051/0004-6361/201732078|issn=0004-6361|s2cid=119395824}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|B}};" |[[天船五]] (位于[[英仙座α星团]])
|2860
| -3.901
|520
| style="background: lightblue;" |3.01
|14900
|{{SIMBAD link|Delta+Persei|SIMBAD}}
|<ref name="XHIP" /><ref name="clpl4" />
|-
| style="background: {{star-color|B}};" |[[心宿二]] B (位于[[本地泡|环泡1]])
|2820
| -3.885
|550
| style="background: lightblue;" |5.5
|18500
|{{SIMBAD link|Alpha+Scorpii+B|SIMBAD}}
|<ref name="antaresb">{{cite journal|last1=Kudritzki|first1=R. P.|last2=Reimers|first2=D.|date=1978|title=On the absolute scale of mass-loss in red giants. II. Circumstellar absorption lines in the spectrum of alpha Sco B and mass-loss of alpha Sco A|journal=Astronomy and Astrophysics|volume=70|page=227|bibcode=1978A&A....70..227K}}</ref><ref name="hr" />
|-
| style="background: {{star-color|B}};" |[[孔雀十一]] (位于[[杜鹃-时钟座星协]])
|2150
| -3.593
|180
| style="background: lightblue;" |1.94
|17700
|{{SIMBAD link|Alpha+Pavonis|SIMBAD}}
|<ref name="aa50_369">{{citation|last1=Jerzykiewicz|first1=M.|title=Empirical Luminosities and Radii of Early-Type Stars after Hipparcos|date=September 2000|journal=Acta Astronomica|volume=50|pages=369–380|bibcode=2000AcA....50..369J|last2=Molenda-Zakowicz|first2=J.}}</ref><ref name="aass34_1">{{citation|last1=Nicolet|first1=B.|title=Photoelectric photometric Catalogue of homogeneous measurements in the UBV System|journal=Astronomy and Astrophysics Supplement Series|volume=34|pages=1–49|year=1978|bibcode=1978A&AS...34....1N}}</ref>
|-
| style="background: {{star-color|B}};" |[[昴宿六]] A (位于[[昴宿星團]])
|1820
| -3.409
|440
| style="background: lightblue;" |2.87
|12300
|{{SIMBAD link|Eta+Tauri|SIMBAD}}
|<ref name="harmanec">{{cite journal|last1=Harmanec|first1=P.|year=2000|title=Physical Properties and Evolutionary Stage of Be Stars|journal=The be Phenomenon in Early-Type Stars|volume=214|page=13|bibcode=2000ASPC..214...13H}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|B}};" |[[天船四]] (位于[[英仙座α星团]])
|775
| -2.483
|580
| style="background: lightblue;" |4.31
|16000
|{{SIMBAD link|Psi+Persei|SIMBAD}}
|<ref name="XHIP" /><ref name="ducati" />
|-
| style="background: {{star-color|B}};" |[[天狼增四]] (位于[[科林德121]])
|715
| -2.397
|440
| style="background: lightblue;" |4.1
|13600
|{{SIMBAD link|Gamma+Canis+Majoris|SIMBAD}}
|<ref name="XHIP" /><ref name="apjss52_7">{{citation|last1=Fernie|first1=J. D.|title=New UBVRI photometry for 900 supergiants|date=May 1983|journal=Astrophysical Journal Supplement Series|volume=52|pages=7–22|postscript=.|bibcode=1983ApJS...52....7F|doi=10.1086/190856}}</ref>
|-
| style="background: {{star-color|B}};" |[[蓋屋一]] (位于[[双鱼-波江座星流]])
|340
| -1.589
|440
| style="background: lightblue;" |4.71
|13500
|{{SIMBAD link|Omicron+Aquarii|SIMBAD}}
|<ref name="XHIP" /><ref name="aj84_1713">{{citation|last1=Feinstein|first1=A.|title=The photometric behavior of Be Stars|date=November 1979|journal=Astronomical Journal|volume=84|pages=1713–1725|postscript=.|bibcode=1979AJ.....84.1713F|doi=10.1086/112600|last2=Marraco|first2=H. G.}}</ref>
|-
| style="background: {{star-color|B}};" |[[天园三]] (位于[[杜鹃-时钟座星协]])
|255
| -1.276
|150
| style="background: lightblue;" |3.55
|13700
|{{SIMBAD link|Phi+Eridani|SIMBAD}}
|<ref name="Mcdonald2012">{{citation|last1=McDonald|first1=I.|title=Fundamental Parameters and Infrared Excesses of Hipparcos Stars|date=2012|journal=Monthly Notices of the Royal Astronomical Society|volume=427|issue=1|pages=343–57|postscript=.|arxiv=1208.2037|bibcode=2012MNRAS.427..343M|doi=10.1111/j.1365-2966.2012.21873.x|display-authors=1|last2=Zijlstra|first2=A. A.|last3=Boyer|first3=M. L.|s2cid=118665352}}</ref><ref name="Mermilliod1986">{{citation|last1=Mermilliod|first1=J.-C.|title=Compilation of Eggen's UBV data, transformed to UBV (unpublished)|date=1986|journal=Catalogue of Eggen's UBV Data|postscript=.|publisher=[[SIMBAD]]|bibcode=1986EgUBV........0M}}</ref>
|-
| style="background: {{star-color|B}};" |[[天炉座ν|天庾一]] (位于[[双鱼-波江座星流]])
|245
| -1.233
|370
| style="background: lightblue;" |4.69
|13400
|{{SIMBAD link|nu+Fornacis|SIMBAD}}
|<ref name="aaa334_181">{{cite journal|last1=North|first1=P.|date=1998|title=Do SI stars undergo any rotational braking?|journal=Astronomy and Astrophysics|volume=334|pages=181–87|arxiv=astro-ph/9802286|bibcode=1998A&A...334..181N}}</ref><ref name="ducati" />
|-
| style="background: {{star-color|B}};" |[[小斗二]] (位于[[天蝎-半人马星协]]内的[[蝘蜓座ε移动星群]])
|100
| -0.26
|360
| style="background: lightblue;" |4.91
|10900
|{{SIMBAD link|Epsilon+Chamaeleontis|SIMBAD}}
|<ref name="Fang2013">{{citation|last1=Fang|first1=M.|title=Young stars in ɛ Chamaleontis and their disks: disk evolution in sparse associations|date=January 2013|url=https://repositorio.uam.es/bitstream/10486/662676/1/young_fang_aa_2013.pdf|journal=Astronomy & Astrophysics|volume=549|page=17|postscript=.|arxiv=1209.5832|bibcode=2013A&A...549A..15F|doi=10.1051/0004-6361/201118528|id=A15|display-authors=1|last2=van Boekel|first2=R.|last3=Bouwman|first3=J.|last4=Henning|first4=Th.|last5=Lawson|first5=W. A.|last6=Sicilia-Aguilar|first6=A.|s2cid=118332644}}</ref><ref name="clpl4" />
|-
| style="background: {{star-color|B}};" |[[蝘蜓座η|小斗七]] (位于[[天蝎-半人马星协]]内的[[蝘蜓座η移动星群]])
|95
| -0.204
|310
| style="background: lightblue;" |5.453
|12500
|{{SIMBAD link|Eta+Chamaeleontis|SIMBAD}}
|<ref name="XHIP" /><ref name="tycho2" />
|-
| style="background: {{star-color|B}};" |[[蛇腹二]] (位于[[杜鹃-时钟座星协]])
|60
|0.295
|150
| style="background: lightblue;" |4.12
|11000
|{{SIMBAD link|Epsilon+Hydri|SIMBAD}}
|<ref name="Zorec2012">{{cite journal|last1=Zorec|first1=J.|last2=Royer|first2=F.|year=2012|title=Rotational velocities of A-type stars|journal=Astronomy & Astrophysics|volume=537|page=A120|arxiv=1201.2052|bibcode=2012A&A...537A.120Z|doi=10.1051/0004-6361/201117691|s2cid=55586789}} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=J/A%2bA/537/A120/table1&HD=16978 Vizier catalog entry] {{Wayback|url=http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=J%2FA%2BA%2F537%2FA120%2Ftable1&HD=16978 |date=20210425141427 }}</ref><ref name="XHIP">{{cite journal|last1=Anderson|first1=E.|last2=Francis|first2=Ch.|year=2012|title=XHIP: An extended hipparcos compilation|journal=Astronomy Letters|volume=38|issue=5|page=331|arxiv=1108.4971|bibcode=2012AstL...38..331A|doi=10.1134/S1063773712050015|s2cid=119257644}} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=V/137D/XHIP&HIP=12394 Vizier catalog entry] {{Wayback|url=http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=V%2F137D%2FXHIP&HIP=12394 |date=20210427175515 }}</ref>
|-
| style="background: {{star-color|B}};" |[[羽林軍二十五]] (位于[[双鱼-波江座星流]])
|50
|0.429
|320
| style="background: lightblue;" |5.66
|10600
|{{SIMBAD link|Tau1+Aquarii|SIMBAD}}
|<ref name="XHIP" /><ref name="mnrassa27_11">{{citation|last1=Corben|first1=P. M.|title=Photoelectric Magnitudes and Colours for Bright Southern Stars|journal=Monthly Notes of the Astronomical Society of Southern Africa|volume=27|page=11|year=1968|postscript=.|bibcode=1968MNSSA..27...11C|last2=Stoy|first2=R. H.}}</ref>
|-
| style="background: {{star-color|B}};" |[[鸟喙四]] A (位于[[杜鹃-时钟座星协]])
|40
|0.735
|140
| style="background: lightblue;" |4.37
|10600
|{{SIMBAD link|Beta1+Tucanae|SIMBAD}}
|<ref>{{citation|last1=Silaj|first1=J.|title=The Hα Profiles of Be Shell Stars|date=November 2014|journal=The Astrophysical Journal|volume=795|issue=1|page=12|postscript=.|bibcode=2014ApJ...795...82S|doi=10.1088/0004-637X/795/1/82|id=82|display-authors=1|last2=Jones|first2=C. E.|last3=Sigut|first3=T. A. A.|last4=Tycner|first4=C.}}</ref><ref name="hr" />
|-
| style="background:lightyellow;" |[[太阳]] (位于[[太阳系]])
|1
|4.739996
|0.0000158
| style="background: lightyellow;" | -26.744
|5772
|{{URL|https://www.iau.org/zhwiki/static/resolutions/IAU2015_English.pdf|IAU}}
|<ref>{{citation|title=International Astronomical Union 2015 RESOLUTION|date=13 August 2015|url=https://www.iau.org/zhwiki/static/resolutions/IAU2015_English.pdf|publisher=International Astronomical Union|accessdate=2021-07-11|archive-date=2016-01-28|archive-url=https://web.archive.org/web/20160128180606/https://www.iau.org/zhwiki/static/resolutions/IAU2015_English.pdf|dead-url=no}}</ref><ref>{{Cite journal|last1=Luzum|first1=Brian|last2=Capitaine|first2=Nicole|last3=Fienga|first3=Agnès|last4=Folkner|first4=William|last5=Fukushima|first5=Toshio|last6=Hilton|first6=James|last7=Hohenkerk|first7=Catherine|last8=Krasinsky|first8=George|last9=Petit|first9=Gérard|last10=Pitjeva|first10=Elena|last11=Soffel|first11=Michael|date=August 2011|title=The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy|url=http://link.springer.com/10.1007/s10569-011-9352-4|journal=Celestial Mechanics and Dynamical Astronomy|volume=110|issue=4|pages=293–304|bibcode=2011CeMDA.110..293L|doi=10.1007/s10569-011-9352-4|issn=0923-2958|doi-access=free}}</ref><ref>{{Cite journal|last1=Bessell|first1=M.S.|last2=Castelli|first2=F.|last3=Plez|first3=B.|date=1998|title=Model atmospheres broad-band colors, bolometric corrections and temperature calibrations for O–M stars|journal=[[Astronomy and Astrophysics]]|volume=333|pages=231–250|bibcode=1998A&A...333..231B}}</ref>
|}
|}


要注意的是即使是最明亮的[[恆星]]（比[[太陽]]明亮四千萬倍）仍然不如像是[[類星體]]，目前已經發現了數百個，這種銀河系外的天體明亮。現在所知最亮的類星體是在[[室女座]]的[[3C 273]]，它的平均[[視星等]]是12.8等（使用[[望遠鏡]]才能看見），但是[[絕對星等]]是-26.7等。如果它在距離地球10[[秒差距]]的位置上，看起來將如同太陽（視星等-26.8）一般的明亮，因此類星體的[[發光度]]是太陽的2兆（10<sup>12</sup>）倍，或是像我們[[銀河系]]這樣的巨型[[星系]]總亮度的100倍。然而也發現類星體的光度在不同的時間週期內也不一樣。
要注意的是即使是最明亮的[[恆星]]（比[[太陽]]明亮四千萬倍）仍然不如像是[[類星體]]，目前已經發現了數百個，這種銀河系外的天體明亮。現在所知最亮的類星體是在[[室女座]]的[[3C 273]]，它的平均[[視星等]]是12.8等（使用[[望遠鏡]]才能看見），但是[[絕對星等]]是-26.7等。如果它在距離地球10[[秒差距]]的位置上，看起來將如同太陽（視星等-26.8）一般的明亮，因此類星體的[[發光度]]是太陽的2兆（10<sup>12</sup>）倍，或是像我們[[銀河系]]這樣的巨型[[星系]]總亮度的100倍。然而也發現類星體的光度在不同的時間週期內也不一樣。


根據[[伽馬射線]]的觀察，一顆被稱為[[SGR 1806-20]]的[[磁星]]（[[中子星]]的一種類型），曾經在2004年12月27日將極端強烈的爆發傳達到地球。它是來自[[太陽系]]外對我們的[[行星]]造成最明亮的衝擊事件。如果[[伽馬射線]]能夠看見，它的光度將達到−29，會比我們的[[太陽]]還要明亮''（如同[[雨燕衛星]]所觀測到的）''.
根據[[伽馬射線]]的觀察，一顆被稱為[[SGR 1806-20]]的[[磁星]]（[[中子星]]的一種類型），曾經在2004年12月27日將極端強烈的爆發傳達到地球。它是來自[[太陽系]]外對我們的[[行星]]造成最明亮的衝擊事件。如果[[伽馬射線]]能夠看見，它的光度將達到−29，會比我們的[[太陽]]還要明亮''（如同[[雨燕衛星]]所觀測到的）''。


在1998年偵測到的[[伽馬射線暴]][[GRB 971214]]在當時被認為是[[宇宙]]間最巨大的能量事件，等同於數百顆[[超新星]]釋出的能量。稍後的研究指出因為幾何的關係射向地球的能量或許相當於一顆超新星將環繞在周圍氣體的總能量集成光束射向地球。
在1998年偵測到的[[伽馬射線暴]][[GRB 971214]]在當時被認為是[[宇宙]]間最巨大的能量事件，等同於數百顆[[超新星]]釋出的能量。稍後的研究指出因為幾何的關係射向地球的能量或許相當於一顆超新星將環繞在周圍氣體的總能量集成光束射向地球。


== 參見 ==
== 參見 ==
{{Portal|恆星
}}

* [[恆星列表]]
* [[恆星列表]]
* [[巨大恆星列表]]
* [[巨大恆星列表]]
第486行： 第2,458行：
* [[伽瑪射線暴]]
* [[伽瑪射線暴]]
* [[類星體]]
* [[類星體]]

== 參考資料 ==
{{Reflist|2}}


== 外部連結 ==
== 外部連結 ==


* [http://www.rssd.esa.int/SA-general/Projects/Hipparcos/table364.html The 150 Most Luminous Stars in the Hipparcos Catalogue]
* [http://www.rssd.esa.int/SA-general/Projects/Hipparcos/table364.html The 150 Most Luminous Stars in the Hipparcos Catalogue] {{Wayback|url=http://www.rssd.esa.int/SA-general/Projects/Hipparcos/table364.html |date=20090122083419 }}
* [http://www.spaceref.com/news/viewpr.html?pid=13334 About LBV 1806-20]
* [http://www.spaceref.com/news/viewpr.html?pid=13334 About LBV 1806-20] {{Wayback|url=http://www.spaceref.com/news/viewpr.html?pid=13334 |date=20190912030517 }}
* [http://www.astronomynotes.com/starprop/s4.htm The Magnitude system]
* [http://www.astronomynotes.com/starprop/s4.htm The Magnitude system]{{Wayback|url=http://www.astronomynotes.com/starprop/s4.htm |date=20180801130342 }}
* [http://csep10.phys.utk.edu/astr162/lect/stars/magnitudes.html About stellar magnitudes]
* [http://csep10.phys.utk.edu/astr162/lect/stars/magnitudes.html About stellar magnitudes] {{Wayback|url=http://csep10.phys.utk.edu/astr162/lect/stars/magnitudes.html |date=20200512175551 }}
* [http://www.tim-thompson.com/bright-stars.html Tim Thompson's list of Brightest Star candidates]
* [http://www.tim-thompson.com/bright-stars.html Tim Thompson's list of Brightest Star candidates] {{Wayback|url=http://www.tim-thompson.com/bright-stars.html |date=20090227081515 }}

{{恒星}}


[[Category:恆星列表]]
[[Category:恆星列表]]

2022年10月20日 (四) 23:22的最新版本

下面的恆星列表是依據恆星的絕對熱星等增加（發光度減弱）的順序排列。絕對星等是恆星在距離地球10秒差距所呈現的視星等。絕對熱星等是測量恆星的發光度–一顆恆星每秒鐘所輻射的總能量。這個表并不十分完整，因為一顆恆星的距離如果遠到我們看不到它，我們就無從得知它的發光度。一些參考資料所給的恆星發光度非常的不一樣（不同的順序或不同的恆星），這些恆星的不同數據資料有些不見得是不可靠，而是注意的和分析時注重的物理資訊不同和有實際上的困難。

图例
沃尔夫-拉叶星
高光度蓝变星
O型星
B型星

太陽光度1百萬倍以上的恒星：

恒星名称 輻射熱光度(太陽=1) 絕對熱星等 距離(光年) 视星等 有效温度(K) 链接 參考文獻
R136a1 (位于大麦哲伦星系内的蜘蛛星云) 6166000 -12.235 163000 12.28 46000 SIMBAD [1][2]
R136a2 (位于大麦哲伦星系内的蜘蛛星云) 5623000 -12.135 163000 12.34 50000 SIMBAD [1][2]
BAT99-98 (位于大麦哲伦星系内的蜘蛛星云) 5012000 -12.01 165000 13.38 45000 SIMBAD [3][2]
G0.238-0.071 (位于银心) 5012000 -12.01 26000 14.37 (J波段) 39500-44000 SIMBAD [4][5]
M33-013406.63 A (位于三角座星系) 4677000 -11.935 3000000 16.084 30000 SIMBAD [6][7]
海山二 A (位于船底座星云内的川普勒16) 4600000 -11.917 7500 4.3 9400-35200 SIMBAD [8][9]
R136a3 (位于大麦哲伦星系内的蜘蛛星云) 4266000 -11.835 163000 12.97 50000 SIMBAD [1][2]
Sk -69° 249 A (位于大麦哲伦星系内的NGC 2074) 4130000 -11.8 160000 10.68 38900 SIMBAD [10][11]
人马座V4998 (靠近五合星团) 3981000 -11.76 25000 12.534 (J波段) 12000 SIMBAD [12][13]
R136c (位于大麦哲伦星系内的蜘蛛星云) 3802000 -11.71 163000 13.43 51000 SIMBAD [14][2]
BAT99-105 (位于大麦哲伦星系内的蜘蛛星云) 3631000 -11.66 163000 12.78 47300 SIMBAD [15][2]
默瑟23-2 (位于靠近银河平面的默瑟23) 3631000 -11.66 21200 8.646 (J波段) 38000 SIMBAD [16][13]
G0.070+0.025 (位于银心) 3311000 -11.56 26000 14.799 (J波段) 45000 SIMBAD [4]
手枪星 (位于五合星团) 3300000 -11.556 25000 11.79 (J波段) 11800 SIMBAD [17][18]
默瑟30-1 A (位于龙鱼星云内的默瑟30) 3236000 -11.535 40000 10.33 (J波段) 32200 SIMBAD [19]
VFTS 682 (位于大麦哲伦星系内的蜘蛛星云) 3236000 -11.535 164000 16.08 52200 SIMBAD [15][2]
WR 42e (位于NGC 3603内的HD 97950) 3200000 -11.523 25000 14.53 43000 SIMBAD [20]
牡丹星 (靠近银心) 3162000 -11.51 26000 12.978 (J波段) 25100 SIMBAD [21][13]
R99 (位于大麦哲伦星系内的N44) 3162000 -11.51 163000 11.52 28000 SIMBAD [3][22]
Var A-1 (位于仙女座星系) 3133000 -11.5 2500000 17.143 20400-28100 SIMBAD [23][7]
VFTS 1022 (位于大麦哲伦星系内的蜘蛛星云) 3020000 -11.46 164000 13.47 42200 SIMBAD [15][2]
WR 24 (位于船底座星云的科林德228) 2951000 -11.435 8200 6.48 50100 SIMBAD [24][25]
CXOGC J174528.6-285605 (位于银心) 2884000 -11.41 26000 14.46 (J波段) 30000 SIMBAD [26]
G0.059-0.068 (位于银心) 2884000 -11.41 26000 13.337 (J波段) 39500-44000 SIMBAD [4][5]
HD 97950 B (位于NGC 3603内的HD 97950) 2884000 -11.41 24000 11.33 42000 SIMBAD [27][28]
BAT99-116 A (位于大麦哲伦星系内的蜘蛛星云) 2692000 -11.335 163000 13.09 53000 SIMBAD [29][2]
WR 102hb (位于五合星团) 2630000 -11.31 26000 13.9 (J波段) 25100 SIMBAD [30][18]
BAT99-80 A (位于大麦哲伦星系内的NGC 2044) 2512000 -11.26 165000 13 45000 SIMBAD [3][31]
R146 (位于大麦哲伦星系内的蜘蛛星云) 2512000 -11.26 164000 13.11 63000 SIMBAD [3][2]
VFTS 482 (位于大麦哲伦星系内的蜘蛛星云) 2512000 -11.26 164000 12.95 42200 SIMBAD [15][2]
HD 97950 A1a (位于NGC 3603内的HD 97950) 2455000 -11.235 24000 11.18 42000 SIMBAD [27][28]
WR 102ea (位于五合星团) 2455000 -11.235 26000 13.18 (J波段) 25100 SIMBAD [30][18]
CXOGC J174516.1-284909 (位于银心) 2399000 -11.21 26000 11.49 (J波段) 20000 SIMBAD [26]
CXOGC J174711.4-283006 (位于银心) 2399000 -11.21 26000 16.56 (J波段) 30000 SIMBAD [26]
WR 25 A (位于船底座星云内的川普勒16) 2399000 -11.21 6800 8.8 50100 SIMBAD [24][22]
LGGS J004444.52+412804.0 (位于仙女座星系) 2377000 -11.2 2500000 18.1 7000-18000 SIMBAD [23][32]
Sk -69° 212 (位于大麦哲伦星系内的NGC 2044) 2377000 -11.2 160000 12.416 45400 SIMBAD [10][33]
WR 93 (位于NGC 6357内的匹斯密斯24) 2377000 -11.2 5700 10.68 71000 SIMBAD [34][22]
BAT99-116 B (位于大麦哲伦星系内的蜘蛛星云) 2344000 -11.185 163000 13.09 53000 SIMBAD [29][2]
VVV CL041-8 (位于VVV CL041) 2344000 -11.185 13700 10.146 (J波段) 34000 SIMBAD [35][13]
Cl 1813-178 #16 (位于W33分子云内的Cl 1813-178) 2291000 -11.16 15300 9.428 (J波段) 30200 SIMBAD [36][13]
VVV CL074-12 (位于VVV CL074) 2291000 -11.16 20000 12.34 (J波段) 22500 SIMBAD [37]
圆拱星团-F6 (位于圆拱星团) 2239000 -11.135 25000 15.75 (J波段) 33900 SIMBAD [38][39]
圆拱星团-F9 (位于圆拱星团) 2239000 -11.135 25000 16.1 (J波段) 36600 SIMBAD [38][39]
HD 5980 A (位于小麦哲伦星系内的NGC 346) 2239000 -11.135 200000 11.31 21000-53000 SIMBAD [40][41]
HD 97950 C1 (位于NGC 3603内的HD 97950) 2239000 -11.135 24000 11.89 44000 SIMBAD [27][28]
R136b (位于大麦哲伦星系内的蜘蛛星云) 2239000 -11.135 165000 13.24 37000 SIMBAD [1][2]
R145 A (位于大麦哲伦星系内的蜘蛛星云) 2239000 -11.135 163000 12.04 50000 SIMBAD [42][2]
Var 83 (位于三角座星系) 2239000 -11.135 3000000 16.027 18000-37000 SIMBAD [43][44]
CXOGC J174712.2-283121 (位于银心) 2188000 -11.11 26000 17.06 (J波段) 35000 SIMBAD [26]
HD 269810 (位于大麦哲伦星系内的NGC 2032) 2188000 -11.11 170000 12.22 52500 SIMBAD [45][11]
VFTS 1021 (位于大麦哲伦星系内的蜘蛛星云) 2188000 -11.11 164000 13.35 39800 SIMBAD [15][2]
ST5-31 (位于大麦哲伦星系内的NGC 2074) 2168000 -11.1 160000 12.273 50700 SIMBAD [10][46]
G0.058+0.014 (位于银心) 2138000 -11.085 26000 14.704 (J波段) 45000 SIMBAD [4]
HSH95-36 (位于大麦哲伦星系内的蜘蛛星云) 2138000 -11.085 163000 14.41 52000 SIMBAD [1][2]
R145 B (位于大麦哲伦星系内的蜘蛛星云) 2138000 -11.085 163000 12.04 43000 SIMBAD [42][2]
WR 89 (位于HM 1) 2138000 -11.085 9500 11.02 39800 SIMBAD [24][11]
AFGL 2298 (靠近银河平面) 2000000 -11.013 33000 12.164 (J波段) 15500-26000 SIMBAD [47][13]
圆拱星团-F1 (位于圆拱星团) 1995000 -11.01 25000 16.3 (J波段) 33200 SIMBAD [38][39]
圆拱星团-F4 (位于圆拱星团) 1995000 -11.01 25000 15.63 (J波段) 36800 SIMBAD [38][39]
圆拱星团-F7 (位于圆拱星团) 1995000 -11.01 25000 15.74 (J波段) 32900 SIMBAD [38][39]
CXOGC J174656.3-283232 (位于银心) 1995000 -11.01 26000 16.74 (J波段) 30000 SIMBAD [26]
LBV 1806-20 (位于银心内的G10.0–0.3) 1995000 -11.01 28000 13.66 (J波段) 18000-32000 SIMBAD [48][13]
默瑟81-2 (位于G338.4+0.2内的默瑟81) 1995000 -11.01 35900 13.25 (J波段) 36000 SIMBAD [49]
VFTS 545 (位于大麦哲伦星系内的蜘蛛星云) 1995000 -11.01 164000 13.32 47300 SIMBAD [15][2]
WR 147S (位于天鹅座OB2) 1995000 -11.01 5800 13.86 39800 SIMBAD [24][50]
DBSB 179-15 (位于G347.6+0.2内的DBSB 179) 1950000 -10.985 25800 12.5 (J波段) 37000 SIMBAD [51][52]
G0.114+0.021 (位于银心) 1950000 -10.985 26000 16.672 (J波段) 40000 SIMBAD [4]
R136a5 (位于大麦哲伦星系内的蜘蛛星云) 1950000 -10.985 165000 13.71 47000 SIMBAD [1][2]
AB6 A (位于小麦哲伦星系内的NGC 371) 1905000 -10.96 197000 12.3 80000 SIMBAD [40][53]
R136a8 (位于大麦哲伦星系内的蜘蛛星云) 1905000 -10.96 165000 14.42 51000 SIMBAD [54][2]
WR 22 A (位于船底座星云的波鸿10) 1905000 -10.96 8200 6.42 44700 SIMBAD [24][22]
R136a6 (位于大麦哲伦星系内的蜘蛛星云) 1862000 -10.935 165000 13.35 53000 SIMBAD [1][2]
Hen 3-519 (位于蓝泡泡星云) 1820000 -10.91 24000 10.85 30200 SIMBAD [55][41]
LGGS J004051.59+403303.0 (位于仙女座星系) 1803000 -10.9 2500000 16.989 18000-24000 SIMBAD [23][7]
MSX5C G358.5391+00.1305 (位于Wray 17-96) 1800000 -10.898 15000 15 13000 SIMBAD [56][11]
HD 5980 B (位于小麦哲伦星系内的NGC 346) 1778000 -10.885 200000 11.31 45000 SIMBAD [40][28]
R136a7 (位于大麦哲伦星系内的蜘蛛星云) 1778000 -10.885 165000 13.97 49000 SIMBAD [1][2]
WR 130 (位于天鹅座OB3) 1778000 -10.885 21700 12.13 44700 SIMBAD [24][11]
WR 21a A (来自维斯特卢2的速逃星) 1778000 -10.885 14300 12.661 45000 SIMBAD [57][11]
人马座V4650 (位于五合星团) 1770000 -10.88 25000 12.31 (J波段) 11300 SIMBAD [58][18]
CXOGC J174536.1-285638 (位于银心) 1738000 -10.86 26000 15.55 (J波段) 30000 SIMBAD [26]
默瑟30-7 A (位于龙鱼星云内的默瑟30) 1738000 -10.86 40000 11.516 (J波段) 41400 SIMBAD [19]
R136a4 (位于大麦哲伦星系内的蜘蛛星云) 1738000 -10.86 165000 13.41 48000 SIMBAD [1][2]
VFTS 506 (位于大麦哲伦星系内的蜘蛛星云) 1738000 -10.86 164000 13.31 47300 SIMBAD [15][2]
DBSB 179-20 (位于G347.6+0.2内的DBSB 179) 1698000 -10.835 25800 12.37 (J波段) 35000 SIMBAD [51][52]
R147 (位于大麦哲伦星系内的蜘蛛星云) 1698000 -10.835 164000 13.02 50000 SIMBAD [3][2]
VFTS 16 (位于大麦哲伦星系内的蜘蛛星云) 1698000 -10.835 164000 13.55 53100 SIMBAD [15][2]
天鹅座OB2-12 A (位于天鹅座OB2) 1660000 -10.81 5000 11.702 13700 SIMBAD [59][60]
Sher 18 (位于NGC 3603内的HD 97950) 1644000 -10.8 25000 12.51 39500 SIMBAD [28][61]
Sher 47 (位于NGC 3603内的HD 97950) 1644000 -10.8 25000 12.67 44000 SIMBAD [28][61]
Mercer 23-1 (位于靠近银河平面的默瑟23) 1622000 -10.785 21200 10.615 (J波段) 35000 SIMBAD [16][13]
VFTS 1017 (位于大麦哲伦星系内的蜘蛛星云) 1622000 -10.785 164000 14.52 50100 SIMBAD [15][2]
WR 87 (位于HM 1) 1622000 -10.785 9500 11.83 44700 SIMBAD [24][11]
仙女座AF (位于仙女座星系) 1585000 -10.76 2500000 17.325 28000 SIMBAD [43][7]
圆拱星团-F12 (位于圆拱星团) 1585000 -10.76 25000 16.4 (J波段) 36900 SIMBAD [38][39]
HSH95-18 (位于大麦哲伦星系内的蜘蛛星云) 1585000 -10.76 163000 13.87 47000 SIMBAD [2]
LHO 110 (位于五合星团) 1585000 -10.76 26000 13.87 (J波段) 25100 SIMBAD [30][18]
R140a1 (位于大麦哲伦星系内的蜘蛛星云) 1585000 -10.76 163000 12.12 34000 SIMBAD [2]
VFTS 457 (位于大麦哲伦星系内的蜘蛛星云) 1585000 -10.76 164000 13.74 39800 SIMBAD [15][2]
WR 107 (位于人马座OB1) 1585000 -10.76 9400 13.51 50100 SIMBAD [24][11]
WR 140 B (位于天鹅座OB1) 1585000 -10.76 5300 6.85 35000 SIMBAD [62][22]
WR 148 A (来自银河平面的速逃星) 1585000 -10.76 27100 10.3 39800 SIMBAD [24][22]
CXOGC J174617.0-285131 (位于银心) 1549000 -10.735 26000 14.98 (J波段) 40000 SIMBAD [26]
CXOGC J174725.3-282709 (位于银心) 1549000 -10.735 26000 16.37 (J波段) 30000 SIMBAD [26]
Sk -68° 137 (位于大麦哲伦星系内的蜘蛛星云) 1549000 -10.735 160000 13.346 55000 SIMBAD [45][33]
WR 102i (位于五合星团) 1549000 -10.735 26000 14.31 (J波段) 31600 SIMBAD [30][18]
HD 97950 A1b (位于NGC 3603内的HD 97950) 1514000 -10.71 24000 11.18 40000 SIMBAD [27][28]
布雷21 A (位于大麦哲伦星系内的NGC 1910) 1500000 -10.7 165000 11.29 71000 SIMBAD [10][11]
HD 97950 A2 (位于NGC 3603内的HD 97950) 1500000 -10.7 24000 12.53 46500 SIMBAD [28][61]
HM 1-6 (位于HM 1) 1500000 -10.7 11000 11.64 44700 SIMBAD [34][63]
LGGS J013245.41+303858.3 (位于三角座星系) 1500000 -10.7 3000000 17.612 34000 SIMBAD [64][7]
NGC 346-W1 (位于小麦哲伦星系内的NGC 346) 1500000 -10.7 200000 12.57 43400 SIMBAD [10][53]
Sk -65° 47 (位于大麦哲伦星系内的NGC 1923) 1500000 -10.7 160000 12.466 47800 SIMBAD [10][33]
Sk 80 (位于小麦哲伦星系内的NGC 346) 1500000 -10.7 200000 12.31 38900 SIMBAD [10][65]
HD 93129 Aa (位于船底座星云内的川普勒14) 1479000 -10.685 7500 6.9 42500 SIMBAD [66][22]
HSH95-46 (位于大麦哲伦星系内的蜘蛛星云) 1445000 -10.66 163000 14.56 49000 SIMBAD [1][2]
VFTS 542 (位于大麦哲伦星系内的蜘蛛星云) 1445000 -10.66 164000 13.49 44700 SIMBAD [15][2]
AB8 A (位于小麦哲伦星系内的NGC 602) 1413000 -10.635 197000 12.9 141000 SIMBAD [40][67]
圆拱星团-F15 (位于圆拱星团) 1413000 -10.635 25000 16.12 (J波段) 35600 SIMBAD [38][39]
CXOGC J174550.2-284911 (位于银心) 1413000 -10.635 26000 15.24 (J波段) 30000 SIMBAD [26]
DBSB 179-4 (位于G347.6+0.2内的DBSB 179) 1413000 -10.635 25800 12.25 (J波段) 30000 SIMBAD [51][52]
LGGS J013235.25+303017.6 (位于三角座星系) 1413000 -10.635 3000000 18.007 33000 SIMBAD [6][68]
R134 (位于大麦哲伦星系内的蜘蛛星云) 1413000 -10.635 164000 12.58 47000 SIMBAD [3][2]
剑鱼座S (位于大麦哲伦星系内的NGC 1910) 1413000 -10.635 169000 10.25 20000 SIMBAD [69][11]
WR 66 (位于圆规座OB1) 1413000 -10.635 16900 11.34 44700 SIMBAD [24][22]
HD 37974 (位于大麦哲伦星系内的N135) 1400000 -10.625 163000 10.99 22500 SIMBAD [70][11]
VFTS 621 (位于大麦哲伦星系内的蜘蛛星云) 1380000 -10.61 164000 15.39 54000 SIMBAD [15][2]
WR 131 (位于天鹅座OB3) 1380000 -10.61 22600 12.08 44700 SIMBAD [24][63]
Sk -69° 104 (位于大麦哲伦星系内的NGC 1910) 1368000 -10.6 160000 12.1 39900 SIMBAD [10][33]
默瑟30-6a A (位于龙鱼星云内的默瑟30) 1349000 -10.585 40000 10.39 (J波段) 29900 SIMBAD [19]
VFTS 427 (位于大麦哲伦星系内的蜘蛛星云) 1349000 -10.585 164000 13.76 39800 SIMBAD [15][2]
CXOGC J174502.8-290859 (位于银心) 1318000 -10.56 26000 13.93 (J波段) 33000 SIMBAD [26]
WR 18 (位于船底座星云内的船底座OB1) 1288000 -10.535 12450 10.83 112200 SIMBAD [24][11]
AB7 A (位于小麦哲伦星系内的NGC 371) 1259000 -10.51 197000 13.016 105000 SIMBAD [40][53]
圆拱星团-F3 (位于圆拱星团) 1259000 -10.51 25000 16.06 (J波段) 29600 SIMBAD [38][39]
圆拱星团-F8 (位于圆拱星团) 1259000 -10.51 25000 16.31 (J波段) 32900 SIMBAD [38][39]
HD 50064 (位于NGC 2301) 1259000 -10.51 9500 8.21 13500 SIMBAD [71]
HSH95-16 (位于大麦哲伦星系内的蜘蛛星云) 1259000 -10.51 163000 13.65 42000 SIMBAD [2]
HSH95-20 (位于大麦哲伦星系内的蜘蛛星云) 1259000 -10.51 164000 13.71 46000 SIMBAD [2]
R139 A (位于大麦哲伦星系内的蜘蛛星云) 1259000 -10.51 163000 11.94 34000 SIMBAD [72][2]
VFTS 259 (位于大麦哲伦星系内的蜘蛛星云) 1259000 -10.51 164000 13.65 37700 SIMBAD [15][2]
VFTS 1031 (位于大麦哲伦星系内的蜘蛛星云) 1259000 -10.51 164000 13.89 48000 SIMBAD [2]
Sk -69° 194 (位于大麦哲伦星系内的NGC 2033) 1247000 -10.5 160000 12.131 45000 SIMBAD [10][73]
ST2-22 (位于大麦哲伦星系内的NGC 2044) 1247000 -10.5 160000 14.3 51300 SIMBAD [10][31]
川普勒27-27 (位于川普勒27) 1247000 -10.5 8200 13.31 37000 SIMBAD [34][11]
HSH95-47 (位于大麦哲伦星系内的蜘蛛星云) 1230000 -10.485 163000 14.72 47000 SIMBAD [1][2]
VFTS 1028 (位于大麦哲伦星系内的蜘蛛星云) 1230000 -10.485 164000 13.84 47300 SIMBAD [15][2]
LH 10-3601 (位于大麦哲伦星系内的NGC 1763) 1202000 -10.46 160000 13.491 55000 SIMBAD [45][33]
AB1 (位于小麦哲伦星系内的DEM S10) 1175000 -10.435 197000 15.238 79000 SIMBAD [74][53]
BI 253 (来自大麦哲伦星系内的蜘蛛星云的速逃星) 1175000 -10.435 164000 13.76 54000 SIMBAD [14][75]
LGGS J013248.26+303950.4 (位于三角座星系) 1175000 -10.435 3000000 17.25 23000 SIMBAD [6][76]
默瑟30-8 (位于龙鱼星云内的默瑟30) 1175000 -10.435 40000 11.658 (J波段) 38100 SIMBAD [19]
NGC 346-W3 (位于小麦哲伦星系内的NGC 346) 1175000 -10.435 200000 12.8 52500 SIMBAD [45][53]
WR 102d (位于五合星团) 1175000 -10.435 26000 15.18 (J波段) 35100 SIMBAD [30][18]
WR 126 (位于狐狸座OB2) 1175000 -10.435 24680 13.29 63000 SIMBAD [77][11]
WR 20a A (位于维斯特卢2) 1150000 -10.412 20000 13.28 43000 SIMBAD [78]
WR 20a B (位于维斯特卢2) 1150000 -10.412 20000 13.28 43000 SIMBAD [78]
GCIRS 16SW A (位于银心) 1149000 -10.411 26000 15.5 (J波段) 24400 SIMBAD [79]
GCIRS 16SW B (位于银心) 1149000 -10.411 26000 15.5 (J波段) 23500 SIMBAD [79]
BAT99-104 (位于大麦哲伦星系内的蜘蛛星云) 1148000 -10.41 165000 14.52 63000 SIMBAD [3][2]
CXOGC J174516.7-285824 (位于银心) 1148000 -10.41 26000 16.67 (J波段) 35000 SIMBAD [26]
G0.121-0.099 (位于银心) 1148000 -10.41 26000 14.972 (J波段) 40000 SIMBAD [4]
G359.797+0.037 (位于银心) 1148000 -10.41 26000 16.1 (J波段) 30000 SIMBAD [4]
HD 93205 A (位于船底座星云内的川普勒16) 1148000 -10.41 7500 7.75 51300 SIMBAD [80][22]
WR 158 (位于仙后座OB1) 1148000 -10.41 16300 11.282 44700 SIMBAD [24][60]
WR 28 (位于FSR 1555) 1148000 -10.41 18700 12.98 50100 SIMBAD [24][11]
HD 303308 (位于船底座星云内的川普勒16) 1138000 -10.4 7500 8.17 51300 SIMBAD [34][22]
M33C-15235 (位于三角座星系) 1138000 -10.4 3000000 17.73 29200 SIMBAD [64][81]
AB9 (位于小麦哲伦星系内的DEM S80) 1122000 -10.385 197000 15.431 100000 SIMBAD [74][53]
圆拱星团-F18 (位于圆拱星团) 1122000 -10.385 25000 16.7 (J波段) 36900 SIMBAD [38][39]
BAT99-64 A (位于大麦哲伦星系内的NGC 2033) 1122000 -10.385 165000 14.073 71000 SIMBAD [3][33]
HSH95-48 (位于大麦哲伦星系内的蜘蛛星云) 1122000 -10.385 163000 14.75 49000 SIMBAD [1][2]
Var B (位于三角座星系) 1122000 -10.385 3000000 16.208 9000 SIMBAD [43][7]
VFTS 562 (位于大麦哲伦星系内的蜘蛛星云) 1122000 -10.385 164000 13.66 42200 SIMBAD [15][2]
WR 37 (位于G291.27-0.71内的SFC 27) 1122000 -10.385 21900 16 100000 SIMBAD [24][11]
VFTS 512 (位于大麦哲伦星系内的蜘蛛星云) 1096000 -10.36 164000 14.28 47700 SIMBAD [15][2]
默瑟30-6b (位于龙鱼星云内的默瑟30) 1072000 -10.335 40000 14.25 (J波段) 30500 SIMBAD [19]
VFTS 3 (位于大麦哲伦星系内的蜘蛛星云) 1072000 -10.335 164000 11.56 21000 SIMBAD [14][2]
VFTS 151 (位于大麦哲伦星系内的蜘蛛星云) 1072000 -10.335 164000 14.13 42200 SIMBAD [15][2]
VFTS 603 (位于大麦哲伦星系内的蜘蛛星云) 1060000 -10.323 164000 13.99 43400 SIMBAD [82][2]
CXOGC J174532.7-285126 (位于银心) 1047000 -10.31 26000 10.72 (J波段) 40000 SIMBAD [26]
HD 93403 A (位于船底座星云内的川普勒16) 1047000 -10.31 10000 8.27 39300 SIMBAD [83][11]
默瑟30-2 (位于龙鱼星云内的默瑟30) 1047000 -10.31 40000 12.63 (J波段) 21200 SIMBAD [19]
R133 (位于大麦哲伦星系内的蜘蛛星云) 1047000 -10.31 163000 12.49 37600 SIMBAD [15][2]
HD 97950 E (位于NGC 3603内的HD 97950) 1038000 -10.3 24000 13.081 46500 SIMBAD [28][61]
HD 229059 (位于伯克利87) 1038000 -10.3 3200 8.7 26300 SIMBAD [34][22]
M33C-10788 (位于三角座星系) 1038000 -10.3 3000000 17.95 32000 SIMBAD [64][81]
Sk -69° 200 (位于大麦哲伦星系内的NGC 2033) 1038000 -10.3 160000 11.18 26300 SIMBAD [10][11]
Sk -69° 259 (位于大麦哲伦星系内的NGC 2081) 1038000 -10.3 160000 11.93 30000 SIMBAD [10][11]
WR 77k (位于维斯特卢1) 1038000 -10.3 11000 18.86 35000 SIMBAD [84][85]
HD 93250 A (位于船底座星云内的川普勒16) 1023000 -10.285 7500 7.5 46000 SIMBAD [86][22]
HSH95-31 (位于大麦哲伦星系内的蜘蛛星云) 1023000 -10.285 163000 14.12 48000 SIMBAD [1][2]
VFTS 267 (位于大麦哲伦星系内的蜘蛛星云) 1023000 -10.285 164000 13.49 44700 SIMBAD [15][2]
VFTS 599 (位于大麦哲伦星系内的蜘蛛星云) 1023000 -10.285 164000 13.8 47300 SIMBAD [14][2]
VVV CL074-9 (位于VVV CL074) 1023000 -10.285 20000 15.22 (J波段) 37000 SIMBAD [37]
WR 156 (位于仙王座OB1) 1023000 -10.285 13400 11.01 39800 SIMBAD [24][41]
圆拱星团-F2 (WR 102aa 位于圆拱星团) 1000000 -10.26 25000 17.84 (J波段) 33500 SIMBAD [38][39]
圆拱星团-F14 (WR 102ba 位于圆拱星团) 1000000 -10.26 25000 16.38 (J波段) 34500 SIMBAD [38][39]
BAT99-68 (位于大麦哲伦星系内的BSDL 2505) 1000000 -10.26 163000 14.13 45000 SIMBAD [3][87]
CXOGC J174628.2-283920 (位于银心) 1000000 -10.26 26000 16.99 (J波段) 40000 SIMBAD [26]
CXOGC J174703.1-283119 (位于银心) 1000000 -10.26 26000 16.23 (J波段) 40000 SIMBAD [26]
HSH95-28 (位于大麦哲伦星系内的蜘蛛星云) 1000000 -10.26 163000 14.09 48000 SIMBAD [2]
HSH95-57 (位于大麦哲伦星系内的蜘蛛星云) 1000000 -10.26 163000 14.8 47000 SIMBAD [2]
R135 A (位于大麦哲伦星系内的蜘蛛星云) 1000000 -10.26 163000 13.48 50000 SIMBAD [3][2]
R140a2 (位于大麦哲伦星系内的蜘蛛星云) 1000000 -10.26 163000 12.12 34000 SIMBAD [2]
R142 (位于大麦哲伦星系内的蜘蛛星云) 1000000 -10.26 163000 11.82 21000 SIMBAD [2]
VFTS 64 (位于大麦哲伦星系内的蜘蛛星云) 1000000 -10.26 164000 14.62 39800 SIMBAD [15][2]
VFTS 591 (位于大麦哲伦星系内的蜘蛛星云) 1000000 -10.26 164000 12.55 27000 SIMBAD [2]
VFTS 1034 (位于大麦哲伦星系内的蜘蛛星云) 1000000 -10.26 164000 13.36 34000 SIMBAD [2]
VVV CL074-3 (位于VVV CL074) 1000000 -10.26 20000 14.72 (J波段) 31500 SIMBAD [37]

一些常见的光度在1百万太阳光度之下的恒星：

恒星名称 輻射熱光度(太陽=1) 絕對熱星等 距離(光年) 视星等 有效温度(K) 链接 參考文獻
尾宿三 (位于天蝎座OB1内的NGC 6231) 851000 -10.085 8210 4.705 17200 SIMBAD [88][89]
弧矢增二十二 (位于船帆座分子云脊内的船帆座R2) 813000 -10.035 1080 2.25 40000 SIMBAD [90][22]
少卫/紫微右垣六 (来自NGC 1502的速逃星) 676000 -9.835 6000 4.29 29000 SIMBAD [86][22]
WR 78 (位于天蝎座OB1内的NGC 6231) 631000 -9.76 4100 6.48 50100 SIMBAD [24][25]
造父三 (来自仙王座OB3的速逃星) 631000 -9.76 3100 5.05 36000 SIMBAD [90][22]
天津增九 (位于天鹅座OB1内的IC 4996) 610000 -9.723 5100 4.82 18700 SIMBAD [91][22]
WR 79a (位于天蝎座OB1内的NGC 6231) 603000 -9.71 5600 5.77 35000 SIMBAD [92][22]
参宿二 (位于猎户座分子云团内的猎户座OB1) 537000 -9.585 2000 1.69 27500 SIMBAD [93][22]
海山二 B (位于船底座星云内的川普勒16) 400000 -9.265 7500 4.3 37200 SIMBAD [94][9]
王良二 (位于仙后座OB14) 302000 -8.96 4000 4.16 23500 SIMBAD [93][22]
弧矢增六 Aa (位于NGC 2362) 299000 -8.95 5120 4.89 32000 SIMBAD [95][22]
天社一 B (位于船帆座OB2) 280000 -8.878 1230 1.83 35000 SIMBAD [96][22]
卷舌三 (位于英仙座OB2内的加州星雲) 263000 -8.81 1200 4.04 35000 SIMBAD [86][22]
参宿一 Aa (位于猎户座分子云团内的猎户座OB1) 250000 -8.755 1260 2.08 29500 SIMBAD [97]
苍蝇座θ Aa (位于半人马座OB1) 234000 -8.685 7400 5.53 83000 SIMBAD [98][22]
军市增五 (位于科林德121) 219000 -8.61 2800 3.043 15500 SIMBAD [99][22]
伐一C1 (位于猎户座分子云团内的猎户四边形星团) 204000 -8.535 1340 5.13 39000 SIMBAD [100][22]
参宿三 Aa1 (位于猎户座分子云团内的猎户座OB1) 191000 -8.46 1200 2.5 29500 SIMBAD [101][102]
天社一 A (位于船帆座OB2) 170000 -8.336 1230 1.83 57000 SIMBAD [96][22]
弧矢二 (位于科林德121) 151000 -8.21 2000 2.45 15000 SIMBAD [93][22]
觜宿一 A (位于猎户座分子云团内的猎户座λ星协) 150000 -8.2 1100 3.54 37700 SIMBAD [103][104]
参宿七 A (位于猎户座分子云团内的猎户座OB1) 120000 -7.96 860 0.13 12100 SIMBAD [105][22]
伐二 A (位于猎户座分子云团内的猎户座OB1) 107000 -7.833 1500 5.02 34900 SIMBAD [106][107]
天市右垣十一/韩 (位于天蝎-半人马星协内的上天蝎次集团) 74100 -7.435 370 2.569 34000 SIMBAD [86][22]
伐三 Aa1 (位于猎户座分子云团内的NGC 1980) 68000 -7.341 1340 2.77 32500 SIMBAD [108][109]
参宿增三十六 (位于猎户座分子云团内的猎户座OB1) 60000 -7.205 2900 4.618 33400 SIMBAD [110][111]
参宿六 (位于猎户座分子云团内的猎户座OB1) 57000 -7.147 650 2.09 26500 SIMBAD [95][22]
天津增二十八 (位于天鹅座OB4) 52000 -7.06 3260 4.233 10800 SIMBAD [112][113]
卷舌四 (位于英仙座OB2) 47000 -6.941 750 2.86 20800 SIMBAD [95][22]
屎 (来自猎户四边形星团的速逃星) 46000 -6.91 1300 5.18 33000 SIMBAD [114][22]
参宿增一 Aa (位于猎户座分子云团内的猎户座OB1) 41700 -6.81 1260 4.07 35000 SIMBAD [115][116]
房宿三 A (位于天蝎-半人马星协内的上天蝎次集团) 38000 -6.71 440 2.307 27400 SIMBAD [117][118]
卷舌二 A (位于英仙座α星团) 28300 -6.391 640 2.88 26500 SIMBAD [95][119]
南船三 A (位于天蝎-半人马星协内的IC 2602) 25700 -6.284 460 2.76 31000 SIMBAD [95][120]
军市一 (位于本地泡) 25000 -6.26 490 1.985 23200 SIMBAD [121][122]
参宿增一 Ab (位于猎户座分子云团内的猎户座OB1) 18600 -5.934 1260 4.07 29000 SIMBAD [115][116]
参宿增一 B (位于猎户座分子云团内的猎户座OB1) 15800 -5.757 1260 4.07 31000 SIMBAD [115][116]
伐二 B (位于猎户座分子云团内的猎户座OB1) 12300 -5.485 1500 6.38 29300 SIMBAD [123]
伐三 Aa2 (位于猎户座分子云团内的NGC 1980) 8630 -5.1 1340 2.77 27000 SIMBAD [108][109]
毕宿八 A (位于双鱼-波江座星流) 5800 -4.669 480 3.47 18700 SIMBAD [95][124]
心宿增四 A (位于蛇夫座ρ星云复合体) 4000 -4.285 360 4.63 22000 SIMBAD [125][22]
天船五 (位于英仙座α星团) 2860 -3.901 520 3.01 14900 SIMBAD [126][120]
心宿二 B (位于环泡1) 2820 -3.885 550 5.5 18500 SIMBAD [127][104]
孔雀十一 (位于杜鹃-时钟座星协) 2150 -3.593 180 1.94 17700 SIMBAD [128][109]
昴宿六 A (位于昴宿星團) 1820 -3.409 440 2.87 12300 SIMBAD [129][22]
天船四 (位于英仙座α星团) 775 -2.483 580 4.31 16000 SIMBAD [126][22]
天狼增四 (位于科林德121) 715 -2.397 440 4.1 13600 SIMBAD [126][130]
蓋屋一 (位于双鱼-波江座星流) 340 -1.589 440 4.71 13500 SIMBAD [126][131]
天园三 (位于杜鹃-时钟座星协) 255 -1.276 150 3.55 13700 SIMBAD [132][133]
天庾一 (位于双鱼-波江座星流) 245 -1.233 370 4.69 13400 SIMBAD [134][22]
小斗二 (位于天蝎-半人马星协内的蝘蜓座ε移动星群) 100 -0.26 360 4.91 10900 SIMBAD [135][120]
小斗七 (位于天蝎-半人马星协内的蝘蜓座η移动星群) 95 -0.204 310 5.453 12500 SIMBAD [126][41]
蛇腹二 (位于杜鹃-时钟座星协) 60 0.295 150 4.12 11000 SIMBAD [136][126]
羽林軍二十五 (位于双鱼-波江座星流) 50 0.429 320 5.66 10600 SIMBAD [126][137]
鸟喙四 A (位于杜鹃-时钟座星协) 40 0.735 140 4.37 10600 SIMBAD [138][104]
太阳 (位于太阳系) 1 4.739996 0.0000158 -26.744 5772 IAU [139][140][141]

要注意的是即使是最明亮的恆星（比太陽明亮四千萬倍）仍然不如像是類星體，目前已經發現了數百個，這種銀河系外的天體明亮。現在所知最亮的類星體是在室女座的3C 273，它的平均視星等是12.8等（使用望遠鏡才能看見），但是絕對星等是-26.7等。如果它在距離地球10秒差距的位置上，看起來將如同太陽（視星等-26.8）一般的明亮，因此類星體的發光度是太陽的2兆（1012）倍，或是像我們銀河系這樣的巨型星系總亮度的100倍。然而也發現類星體的光度在不同的時間週期內也不一樣。

根據伽馬射線的觀察，一顆被稱為SGR 1806-20的磁星（中子星的一種類型），曾經在2004年12月27日將極端強烈的爆發傳達到地球。它是來自太陽系外對我們的行星造成最明亮的衝擊事件。如果伽馬射線能夠看見，它的光度將達到−29，會比我們的太陽還要明亮（如同雨燕衛星所觀測到的）。

在1998年偵測到的伽馬射線暴GRB 971214在當時被認為是宇宙間最巨大的能量事件，等同於數百顆超新星釋出的能量。稍後的研究指出因為幾何的關係射向地球的能量或許相當於一顆超新星將環繞在周圍氣體的總能量集成光束射向地球。

參見

[编辑]

參考資料

[编辑]
  1. ^ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 1.11 1.12 Bestenlehner, Joachim M.; Crowther, Paul A.; Caballero-Nieves, Saida M.; Schneider, Fabian R. N.; Simón-Díaz, Sergio; Brands, Sarah A.; De Koter, Alex; Gräfener, Götz; Herrero, Artemio; Langer, Norbert; Lennon, Daniel J.; Maíz Apellániz, Jesus; Puls, Joachim; Vink, Jorick S. The R136 star cluster dissected with Hubble Space Telescope/STIS. II. Physical properties of the most massive stars in R136. Monthly Notices of the Royal Astronomical Society. 2020, 499 (2): 1918. Bibcode:2020MNRAS.499.1918B. S2CID 221640940. arXiv:2009.05136 可免费查阅. doi:10.1093/mnras/staa2801. 
  2. ^ 2.00 2.01 2.02 2.03 2.04 2.05 2.06 2.07 2.08 2.09 2.10 2.11 2.12 2.13 2.14 2.15 2.16 2.17 2.18 2.19 2.20 2.21 2.22 2.23 2.24 2.25 2.26 2.27 2.28 2.29 2.30 2.31 2.32 2.33 2.34 2.35 2.36 2.37 2.38 2.39 2.40 2.41 2.42 2.43 2.44 2.45 2.46 2.47 2.48 2.49 2.50 2.51 2.52 2.53 2.54 2.55 2.56 2.57 2.58 2.59 2.60 Doran, E. I.; Crowther, P. A.; de Koter, A.; Evans, C. J.; McEvoy, C.; Walborn, N. R.; Bastian, N.; Bestenlehner, J. M.; Gräfener, G.; Herrero, A.; Köhler, K.; Maíz Apellániz, J.; Najarro, F.; Puls, J.; Sana, H.; Schneider, F. R. N.; Taylor, W. D.; van Loon, J. Th.; Vink, J. S. The VLT-FLAMES Tarantula Survey. XI. A census of the hot luminous stars and their feedback in 30 Doradus. Astronomy & Astrophysics. 2013, 558 (134): 30. Bibcode:2013A&A...558A.134D. S2CID 118510909. arXiv:1308.3412 可免费查阅. doi:10.1051/0004-6361/201321824. 
  3. ^ 3.00 3.01 3.02 3.03 3.04 3.05 3.06 3.07 3.08 3.09 Hainich, R.; Rühling, U.; Todt, H.; Oskinova, L. M.; Liermann, A.; Gräfener, G.; Foellmi, C.; Schnurr, O.; Hamann, W. -R. The Wolf-Rayet stars in the Large Magellanic Cloud. Astronomy & Astrophysics. 2014, 565: A27. Bibcode:2014A&A...565A..27H. S2CID 55123954. arXiv:1401.5474 可免费查阅. doi:10.1051/0004-6361/201322696. 
  4. ^ 4.0 4.1 4.2 4.3 4.4 4.5 4.6 Mauerhan, J. C.; Cotera, A.; Dong, H.; Morris, M. R.; Wang, Q. D.; Stolovy, S. R.; Lang, C. Isolated Wolf-Rayet Stars and O Supergiants in the Galactic Center Region Identified Via Paschen-α Excess. The Astrophysical Journal. 2010, 725 (1): 188–199. Bibcode:2010ApJ...725..188M. S2CID 20968628. arXiv:1009.2769 可免费查阅. doi:10.1088/0004-637X/725/1/188. 
  5. ^ 5.0 5.1 Dong, H.; Wang, Q. D.; Cotera, A.; Stolovy, S.; Morris, M. R.; Mauerhan, J.; Mills, E. A.; Schneider, G.; Calzetti, D.; Lang, C. Hubble Space Telescope Paschen α survey of the Galactic Centre: data reduction and products: HST/NICMOS Paschen α survey of the GC. Monthly Notices of the Royal Astronomical Society. 2011-10-11, 417 (1): 114–135 [2021-07-11]. Bibcode:2011MNRAS.417..114D. S2CID 11060463. arXiv:1105.1703 可免费查阅. doi:10.1111/j.1365-2966.2011.19013.x. （原始内容存档于2017-07-07）. 
  6. ^ 6.0 6.1 6.2 Kourniotis, M; Kraus, M; Arias, M L; Cidale, L; Torres, A F. On the evolutionary state of massive stars in transition phases in M33. Monthly Notices of the Royal Astronomical Society. 2018-11-01, 480 (3): 3706–3717 [2021-07-11]. Bibcode:2018MNRAS.480.3706K. ISSN 0035-8711. arXiv:1808.00008 可免费查阅. doi:10.1093/mnras/sty2087. （原始内容存档于2022-02-14）. 
  7. ^ 7.0 7.1 7.2 7.3 7.4 7.5 Massey, Philip; Olsen, K. A. G.; Hodge, Paul W.; Strong, Shay B.; Jacoby, George H.; Schlingman, Wayne; Smith, R. C. A Survey of Local Group Galaxies Currently Forming Stars. I. UBVRI Photometry of Stars in M31 and M33. The Astronomical Journal. 2006, 131 (5): 2478–2496 [2021-07-11]. Bibcode:2006AJ....131.2478M. ISSN 0004-6256. S2CID 118865956. arXiv:astro-ph/0602128 可免费查阅. doi:10.1086/503256. （原始内容存档于2020-06-10）. 
  8. ^ Mehner, A.; De Wit, W.-J.; Asmus, D.; Morris, P. W.; Agliozzo, C.; Barlow, M. J.; Gull, T. R.; Hillier, D. J.; Weigelt, G. Mid-infrared evolution of η Carinae from 1968 to 2018. Astronomy & Astrophysics. 2019, 630: L6. Bibcode:2019A&A...630L...6M. S2CID 202149820. arXiv:1908.09154 可免费查阅. doi:10.1051/0004-6361/201936277. 
  9. ^ 9.0 9.1 Hamaguchi, Kenji; Corcoran, Michael F; Pittard, Julian M; Sharma, Neetika; Takahashi, Hiromitsu; Russell, Christopher M. P; Grefenstette, Brian W; Wik, Daniel R; Gull, Theodore R; Richardson, Noel D; Madura, Thomas I; Moffat, Anthony F. J. Non-thermal X-rays from colliding wind shock acceleration in the massive binary Eta Carinae. Nature Astronomy. 2018, 2 (9): 731–736 [2021-07-11]. Bibcode:2018NatAs.tmp...87H. S2CID 126188024. arXiv:1904.09219 可免费查阅. doi:10.1038/s41550-018-0505-1. （原始内容存档于2020-02-23）. 
  10. ^ 10.00 10.01 10.02 10.03 10.04 10.05 10.06 10.07 10.08 10.09 10.10 10.11 Massey, Philip; Waterhouse, Elizabeth; DeGioia-Eastwood, Kathleen. The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster Turnoffs. I. Results from 19 OB Associations in the Magellanic Clouds. The Astronomical Journal. May 2000, 119 (5): 2214–2241 [2021-07-11]. Bibcode:2000AJ....119.2214M. S2CID 16891188. arXiv:astro-ph/0002233 可免费查阅. doi:10.1086/301345. （原始内容存档于2020-10-30）. 
  11. ^ 11.00 11.01 11.02 11.03 11.04 11.05 11.06 11.07 11.08 11.09 11.10 11.11 11.12 11.13 11.14 11.15 11.16 11.17 11.18 Zacharias, N.; Finch, C. T.; Girard, T. M.; Henden, A.; Bartlett, J. L.; et al. VizieR On-line Data Catalog: UCAC4 Catalogue. VizieR On-line Data Catalog: I/322A. July 2012, 1322. Bibcode:2012yCat.1322....0Z. 
  12. ^ Mauerhan, J. C.; Morris, M. R.; Cotera, A.; Dong, H.; Wang, Q. D.; Stolovy, S. R.; Lang, C.; Glass, I. S. Discovery of a Luminous Blue Variable with an Ejection Nebula Near the Quintuplet Cluster. The Astrophysical Journal. 2010, 713 (1): L33–L36. Bibcode:2010ApJ...713L..33M. S2CID 42696538. arXiv:1002.3379 可免费查阅. doi:10.1088/2041-8205/713/1/L33. 
  13. ^ 13.0 13.1 13.2 13.3 13.4 13.5 13.6 13.7 Cutri, R. M.; Skrutskie, M. F.; Van Dyk, S.; Beichman, C. A.; Carpenter, J. M.; Chester, T.; Cambresy, L.; Evans, T.; Fowler, J.; Gizis, J.; Howard, E.; Huchra, J.; Jarrett, T.; Kopan, E. L.; Kirkpatrick, J. D.; Light, R. M.; Marsh, K. A.; McCallon, H.; Schneider, S.; Stiening, R.; Sykes, M.; Weinberg, M.; Wheaton, W. A.; Wheelock, S.; Zacarias, N. VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). VizieR On-line Data Catalog. 2003. Bibcode:2003yCat.2246....0C. 
  14. ^ 14.0 14.1 14.2 14.3 Schneider, F. R. N.; Sana, H.; Evans, C. J.; Bestenlehner, J. M.; Castro, N.; Fossati, L.; Gräfener, G.; Langer, N.; Ramírez-Agudelo, O. H.; Sabín-Sanjulián, C.; Simón-Díaz, S.; Tramper, F.; Crowther, P. A.; de Koter, A.; de Mink, S. E.; Dufton, P. L.; Garcia, M.; Gieles, M.; Hénault-Brunet, V.; Herrero, A.; Izzard, R. G.; Kalari, V.; Lennon, D. J.; Maíz Apellániz, J.; Markova, N.; Najarro, F.; Podsiadlowski, Ph.; Puls, J.; Taylor, W. D.; van Loon, J. Th.; Vink, J. S.; Norman, C. An excess of massive stars in the local 30 Doradus starburst. Science. 2018, 359 (6371): 69–71. Bibcode:2018Sci...359...69S. PMID 29302009. S2CID 206658504. arXiv:1801.03107 可免费查阅. doi:10.1126/science.aan0106. 
  15. ^ 15.00 15.01 15.02 15.03 15.04 15.05 15.06 15.07 15.08 15.09 15.10 15.11 15.12 15.13 15.14 15.15 15.16 15.17 15.18 15.19 15.20 Bestenlehner, J. M.; Gräfener, G.; Vink, J. S.; Najarro, F.; De Koter, A.; Sana, H.; Evans, C. J.; Crowther, P. A.; Hénault-Brunet, V.; Herrero, A.; Langer, N.; Schneider, F. R. N.; Simón-Díaz, S.; Taylor, W. D.; Walborn, N. R. The VLT-FLAMES Tarantula Survey. XVII. Physical and wind properties of massive stars at the top of the main sequence. Astronomy & Astrophysics. 2014, 570: A38. Bibcode:2014A&A...570A..38B. S2CID 118606369. arXiv:1407.1837 可免费查阅. doi:10.1051/0004-6361/201423643. 
  16. ^ 16.0 16.1 Hanson, M. M.; Kurtev, R.; Borissova, J.; Georgiev, L.; Ivanov, V. D.; Hillier, D. J.; Minniti, D. Obscured clusters: III. Follow-up observations of Mercer 23. Astronomy and Astrophysics. June 2010, 516: A35. Bibcode:2010A&A...516A..35H. ISSN 0004-6361. S2CID 53705451. doi:10.1051/0004-6361/200913122 可免费查阅. 
  17. ^ Lau, R. M.; Herter, T. L.; Morris, M. R.; Adams, J. D. Nature Versus Nurture: Luminous Blue Variable Nebulae in and Near Massive Stellar Clusters at the Galactic Center. The Astrophysical Journal. 2014, 785 (2): 120. Bibcode:2014ApJ...785..120L. S2CID 118447462. arXiv:1403.5298 可免费查阅. doi:10.1088/0004-637X/785/2/120. 
  18. ^ 18.0 18.1 18.2 18.3 18.4 18.5 18.6 Clark, J. S.; Lohr, M. E.; Patrick, L. R.; Najarro, F.; Dong, H.; Figer, D. F. An updated stellar census of the Quintuplet cluster. Astronomy & Astrophysics. 2018, 618: A2. Bibcode:2018A&A...618A...2C. ISSN 0004-6361. S2CID 53501337. arXiv:1805.10139 可免费查阅. doi:10.1051/0004-6361/201833041. 
  19. ^ 19.0 19.1 19.2 19.3 19.4 19.5 de la Fuente, D.; Najarro, F.; Borissova, J.; Ramírez Alegría, S.; Hanson, M. M.; Trombley, C.; Figer, D. F.; Davies, B.; Garcia, M.; Kurtev, R.; Urbaneja, M. A.; Smith, L. C.; Lucas, P. W.; Herrero, A. Probing the Dragonfish star-forming complex: the ionizing population of the young massive cluster Mercer 30. Astronomy & Astrophysics. May 2016, 589: A69. Bibcode:2016A&A...589A..69D. ISSN 0004-6361. S2CID 119096455. arXiv:1602.02503 可免费查阅. doi:10.1051/0004-6361/201528004. 
  20. ^ Roman-Lopes, A. A Galactic O2 If*/WN6 star possibly ejected from its birthplace in NGC 3603. Monthly Notices of the Royal Astronomical Society Letters. 2012, 427 (1): L65–L69. Bibcode:2012MNRAS.427L..65R. S2CID 118453639. arXiv:1209.1598 可免费查阅. doi:10.1111/j.1745-3933.2012.01346.x. 
  21. ^ Barniske, A.; Oskinova, L. M.; Hamann, W. -R. Two extremely luminous WN stars in the Galactic center with circumstellar emission from dust and gas. Astronomy and Astrophysics. 2008, 486 (3): 971. Bibcode:2008A&A...486..971B. S2CID 8074261. arXiv:0807.2476 可免费查阅. doi:10.1051/0004-6361:200809568. 
  22. ^ 22.00 22.01 22.02 22.03 22.04 22.05 22.06 22.07 22.08 22.09 22.10 22.11 22.12 22.13 22.14 22.15 22.16 22.17 22.18 22.19 22.20 22.21 22.22 22.23 22.24 22.25 22.26 22.27 22.28 22.29 22.30 22.31 22.32 22.33 22.34 22.35 Ducati, J. R. VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system. CDS/ADC Collection of Electronic Catalogues. 2002, 2237: 0. Bibcode:2002yCat.2237....0D. 
  23. ^ 23.0 23.1 23.2 Sholukhova, O.; Bizyaev, D.; Fabrika, S.; Sarkisyan, A.; Malanushenko, V.; Valeev, A. New Luminous Blue Variables in the Andromeda galaxy. Monthly Notices of the Royal Astronomical Society. 2014, 447 (3): 2459–2467. Bibcode:2015MNRAS.447.2459S. S2CID 118374186. arXiv:1412.5319 可免费查阅. doi:10.1093/mnras/stu2597. 
  24. ^ 24.00 24.01 24.02 24.03 24.04 24.05 24.06 24.07 24.08 24.09 24.10 24.11 24.12 24.13 24.14 24.15 24.16 Sota, A.; Maíz Apellániz, J.; Morrell, N. I.; Barbá, R. H.; Walborn, N. R.; Gamen, R. C.; Arias, J. I.; Alfaro, E. J.; Oskinova, L. M. The Galactic WN stars revisited. Impact of Gaia distances on fundamental stellar parameters. Astronomy & Astrophysics. 2019, A57: 625. Bibcode:2019A&A...625A..57H. S2CID 104292503. arXiv:1904.04687 可免费查阅. doi:10.1051/0004-6361/201834850. 
  25. ^ 25.0 25.1 Samus, N. N.; Durlevich, O. V.; et al. VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013). VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 2009, 1. Bibcode:2009yCat....102025S. 
  26. ^ 26.00 26.01 26.02 26.03 26.04 26.05 26.06 26.07 26.08 26.09 26.10 26.11 26.12 26.13 Mauerhan, J. C.; Muno, M. P.; Morris, M. R.; Stolovy, S. R.; Cotera, A. Near-infrared Counterparts to Chandra X-ray Sources Toward the Galactic Center. II. Discovery of Wolf-Rayet Stars and O Supergiants. The Astrophysical Journal. 10 February 2010, 710 (1): 706–728 [2021-07-11]. Bibcode:2010ApJ...710..706M. ISSN 0004-637X. S2CID 32339182. arXiv:0912.1055 可免费查阅. doi:10.1088/0004-637X/710/1/706. （原始内容存档于2021-04-10）. 
  27. ^ 27.0 27.1 27.2 27.3 Crowther, P. A.; Schnurr, O.; Hirschi, R.; Yusof, N.; Parker, R. J.; Goodwin, S. P.; Kassim, H. A. The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M⊙ stellar mass limit. Monthly Notices of the Royal Astronomical Society. 2010, 408 (2): 731–751. Bibcode:2010MNRAS.408..731C. S2CID 53001712. arXiv:1007.3284 可免费查阅. doi:10.1111/j.1365-2966.2010.17167.x. 
  28. ^ 28.0 28.1 28.2 28.3 28.4 28.5 28.6 28.7 28.8 Melena, Nicholas W.; Massey, Philip; Morrell, Nidia I.; Zangari, Amanda M. The Massive Star Content of NGC 3603. The Astronomical Journal. 2008, 135 (3): 878–891. Bibcode:2008AJ....135..878M. ISSN 0004-6256. S2CID 16765414. arXiv:0712.2621 可免费查阅. doi:10.1088/0004-6256/135/3/878. 
  29. ^ 29.0 29.1 Tehrani, Katie A.; Crowther, Paul A.; Bestenlehner, Joachim M.; Littlefair, Stuart P.; Pollock, A M T.; Parker, Richard J.; Schnurr, Olivier. Weighing Melnick 34: The most massive binary system known. Monthly Notices of the Royal Astronomical Society. 2019, 484 (2): 2692–2710. Bibcode:2019MNRAS.484.2692T. S2CID 119069481. arXiv:1901.04769 可免费查阅. doi:10.1093/mnras/stz147. 
  30. ^ 30.0 30.1 30.2 30.3 30.4 Liermann, A.; Hamann, W. -R.; Oskinova, L. M.; Todt, H.; Butler, K. The Quintuplet cluster. Astronomy & Astrophysics. 2010, 524: A82. Bibcode:2010A&A...524A..82L. S2CID 30091594. arXiv:1011.5796 可免费查阅. doi:10.1051/0004-6361/200912612. 
  31. ^ 31.0 31.1 Schild, H.; Testor, G. Spectral types and UBV magnitudes of stars in the 30 Doradus complex.. Astronomy and Astrophysics Supplement Series. March 1992, 92: 729–748. Bibcode:1992A&AS...92..729S. S2CID 115371295. 
  32. ^ Humphreys, Roberta M.; Weis, Kerstin; Davidson, Kris; Bomans, D. J.; Burggraf, Birgitta. LUMINOUS AND VARIABLE STARS IN M31 AND M33. II. LUMINOUS BLUE VARIABLES, CANDIDATE LBVs, Fe II EMISSION LINE STARS, AND OTHER SUPERGIANTS. The Astrophysical Journal. 2014-07-02, 790 (1): 48 [2021-07-11]. Bibcode:2014ApJ...790...48H. ISSN 0004-637X. S2CID 119177378. arXiv:1407.2259 可免费查阅. doi:10.1088/0004-637X/790/1/48. （原始内容存档于2021-08-24）. 
  33. ^ 33.0 33.1 33.2 33.3 33.4 33.5 Bonanos, A. Z.; Massa, D. L.; Sewilo, M.; Lennon, D. J.; Panagia, N.; Smith, L. J.; Meixner, M.; Babler, B. L.; Bracker, S.; Meade, M. R.; Gordon, K. D. Spitzersage Infrared Photometry of Massive Stars in the Large Magellanic Cloud. The Astronomical Journal. 2009-10-01, 138 (4): 1003–1021 [2021-07-11]. Bibcode:2009AJ....138.1003B. ISSN 0004-6256. S2CID 14056495. arXiv:0905.1328 可免费查阅. doi:10.1088/0004-6256/138/4/1003. （原始内容存档于2020-12-05）. 
  34. ^ 34.0 34.1 34.2 34.3 34.4 Massey, P.; Degioia-Eastwood, K.; Waterhouse, E. The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster Turnoffs. II. Results from 12 Galactic Clusters and OB Associations. The Astronomical Journal. 2001, 121 (2): 1050–1070. Bibcode:2001AJ....121.1050M. S2CID 53345173. arXiv:astro-ph/0010654 可免费查阅. doi:10.1086/318769. 
  35. ^ Chené, A.-N.; Ramírez Alegría, S.; Borissova, J.; O’Leary, E.; Martins, F.; Hervé, A.; Kuhn, M.; Kurtev, R.; Consuelo Amigo Fuentes, P.; Bonatto, C.; Minniti, D. Massive open star clusters using the VVV survey: IV. WR 62-2, a new very massive star in the core of the VVV CL041 cluster. Astronomy & Astrophysics. December 2015, 584: A31. Bibcode:2015A&A...584A..31C. ISSN 0004-6361. S2CID 118707197. arXiv:1510.02539 可免费查阅. doi:10.1051/0004-6361/201525958. 
  36. ^ Messineo, Maria; Davies, Ben; Figer, Donald F.; Kudritzki, R. P.; Valenti, Elena; Trombley, Christine; Najarro, F.; Michael Rich, R. Massive Stars in the Cl 1813-178 Cluster: An Episode Of Massive Star Formation in the W33 Complex. The Astrophysical Journal. 20 May 2011, 733 (1): 41 [2021-07-11]. Bibcode:2011ApJ...733...41M. ISSN 0004-637X. S2CID 118576212. arXiv:1103.4975 可免费查阅. doi:10.1088/0004-637X/733/1/41. （原始内容存档于2021-04-10）. 
  37. ^ 37.0 37.1 37.2 Martins, F.; Chené, A.-N.; Bouret, J.-C.; Borissova, J.; Groh, J.; Ramírez Alegría, S.; Minniti, D. Massive stars in the young cluster VVV CL074. Astronomy & Astrophysics. 2019, 627: A170. Bibcode:2019A&A...627A.170M. ISSN 0004-6361. S2CID 195798873. arXiv:1907.02357 可免费查阅. doi:10.1051/0004-6361/201935605. 
  38. ^ 38.00 38.01 38.02 38.03 38.04 38.05 38.06 38.07 38.08 38.09 38.10 38.11 Martins, F.; Hillier, D. J.; Paumard, T.; Eisenhauer, F.; Ott, T.; Genzel, R. The most massive stars in the Arches cluster. Astronomy and Astrophysics. 2008, 478 (1): 219–233. Bibcode:2008A&A...478..219M. S2CID 7509876. arXiv:0711.0657 可免费查阅. doi:10.1051/0004-6361:20078469. 
  39. ^ 39.00 39.01 39.02 39.03 39.04 39.05 39.06 39.07 39.08 39.09 39.10 39.11 Figer, Donald F.; Najarro, Francisco; Gilmore, Diane; Morris, Mark; Kim, Sungsoo S.; Serabyn, Eugene; McLean, Ian S.; Gilbert, Andrea M.; Graham, James R.; Larkin, James E.; Levenson, N. A. Massive Stars in the Arches Cluster. The Astrophysical Journal. 2002-12-10, 581 (1): 258–275. Bibcode:2002ApJ...581..258F. ISSN 0004-637X. S2CID 119002004. arXiv:astro-ph/0208145 可免费查阅. doi:10.1086/344154. 
  40. ^ 40.0 40.1 40.2 40.3 40.4 Shenar, T.; Hainich, R.; Todt, H.; Sander, A.; Hamann, W.-R.; Moffat, A. F. J.; Eldridge, J. J.; Pablo, H.; Oskinova, L. M.; Richardson, N. D. Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries. Astronomy & Astrophysics. 2016, 1604: A22. Bibcode:2016A&A...591A..22S. S2CID 119255408. arXiv:1604.01022 可免费查阅. doi:10.1051/0004-6361/201527916. 
  41. ^ 41.0 41.1 41.2 41.3 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. The Tycho-2 catalogue of the 2.5 million brightest stars. Astronomy and Astrophysics. 2000, 355: L27. Bibcode:2000A&A...355L..27H. ISBN 0333750888. doi:10.1888/0333750888/2862. 
  42. ^ 42.0 42.1 Shenar, T.; et al. The Tarantula Massive Binary Monitoring project: II. A first SB2 orbital and spectroscopic analysis for the Wolf-Rayet binary R145. Astronomy & Astrophysics. 2016, 598: A85. Bibcode:2017A&A...598A..85S. S2CID 118546102. arXiv:1610.07614 可免费查阅. doi:10.1051/0004-6361/201629621. 
  43. ^ 43.0 43.1 43.2 Szeifert, T.; Humphreys, R. M.; Davidson, K.; Jones, T. J.; Stahl, O.; Wolf, B.; Zickgraf, F.-J. HST and groundbased observations of the 'Hubble-Sandage' variables in M 31 and M 33. Astronomy and Astrophysics. 1996, 314: 131–145. Bibcode:1996A&A...314..131S. 
  44. ^ Massey, Philip; Neugent, Kathryn F.; Smart, Brianna M. A Spectroscopic Survey of Massive Stars in M31 and M33. The Astronomical Journal. 2016-08-19, 152 (3): 62. Bibcode:2016AJ....152...62M. ISSN 1538-3881. S2CID 35672588. arXiv:1604.00112 可免费查阅. doi:10.3847/0004-6256/152/3/62. 
  45. ^ 45.0 45.1 45.2 45.3 Walborn, N. R.; Morrell, N. I.; Howarth, I. D.; Crowther, P. A.; Lennon, D. J.; Massey, P.; Arias, J. I. A CNO Dichotomy among O2 Giant Spectra in the Magellanic Clouds. The Astrophysical Journal. 2004, 608 (2): 1028–1038. Bibcode:2004ApJ...608.1028W. S2CID 16656083. arXiv:astro-ph/0403557 可免费查阅. doi:10.1086/420761. 
  46. ^ Zaritsky, Dennis; Harris, Jason; Thompson, Ian B.; Grebel, Eva K. The Magellanic Clouds Photometric Survey: The Large Magellanic Cloud Stellar Catalog and Extinction Map. The Astronomical Journal. October 2004, 128 (4): 1606–1614 [2021-07-11]. Bibcode:2004AJ....128.1606Z. ISSN 0004-6256. S2CID 119532934. arXiv:astro-ph/0407006 可免费查阅. doi:10.1086/423910. （原始内容存档于2021-06-08）. 
  47. ^ Clark, J. S.; Crowther, P. A.; Larionov, V. M.; Steele, I. A.; Ritchie, B. W.; Arkharov, A. A. Bolometric luminosity variations in the luminous blue variable AFGL2298. Astronomy and Astrophysics. 2009, 507 (3): 1555–1565. Bibcode:2009A&A...507.1555C. S2CID 119187994. arXiv:0909.4160 可免费查阅. doi:10.1051/0004-6361/200912358. 
  48. ^ Abdalla, H.; Abramowski, A.; Aharonian, F.; Ait Benkhali, F.; Akhperjanian, A. G.; Angüner, E. O.; Arrieta, M.; Aubert, P.; Backes, M.; Balzer, A.; Barnard, M.; Becherini, Y.; Becker Tjus, J.; Berge, D.; Bernhard, S.; Bernlöhr, K.; Birsin, E.; Blackwell, R.; Böttcher, M.; Boisson, C.; Bolmont, J.; Bordas, P.; Bregeon, J.; Brun, F.; Brun, P.; Bryan, M.; Bulik, T.; Capasso, M.; Carr, J.; et al. Extended VHE γ-ray emission towards SGR1806−20, LBV 1806−20, and stellar cluster Cl* 1806−20. Astronomy & Astrophysics. 2018, 612: A11. Bibcode:2018A&A...612A..11H. S2CID 118345803. arXiv:1606.05404 可免费查阅. doi:10.1051/0004-6361/201628695. 
  49. ^ Davies, Ben; de la Fuente, Diego; Najarro, Francisco; Hinton, Jim A.; Trombley, Christine; Figer, Donald F.; Puga, Elena. A newly discovered young massive star cluster at the far end of the Galactic Bar: A young cluster at the far end of the Bar. Monthly Notices of the Royal Astronomical Society. 21 January 2012, 419 (3): 1860–1870. Bibcode:2012MNRAS.419.1860D. ISSN 0035-8711. S2CID 59405479. arXiv:1111.2630 可免费查阅. doi:10.1111/j.1365-2966.2011.19840.x. 
  50. ^ Niemela, Virpi S.; Shara, Michael M.; Wallace, Debra J.; Zurek, David R.; Moffat, Anthony F. J. Hubble Space Telescope Detection of Optical Companions of WR 86, WR 146, and WR 147: Wind Collision Model Confirmed. The Astronomical Journal. 1998, 115 (5): 2047–2052 [2021-07-11]. Bibcode:1998AJ....115.2047N. doi:10.1086/300320. （原始内容存档于2020-05-29）. 
  51. ^ 51.0 51.1 51.2 Borissova, J.; Georgiev, L.; Hanson, M. M.; Clarke, J. R. A.; Kurtev, R.; Ivanov, V. D.; Penaloza, F.; Hillier, D. J.; Zsargó, J. Obscured clusters: IV. The most massive stars in [DBS2003] 179. Astronomy & Astrophysics. October 2012, 546: A110. Bibcode:2012A&A...546A.110B. ISSN 0004-6361. S2CID 119303823. arXiv:1209.6370 可免费查阅. doi:10.1051/0004-6361/201118348. 
  52. ^ 52.0 52.1 52.2 Borissova, J.; Ivanov, V. D.; Hanson, M. M.; Georgiev, L.; Minniti, D.; Kurtev, R.; Geisler, D. The young Galactic star cluster [DBS2003] 179. Astronomy & Astrophysics. September 2008, 488 (1): 151–159. Bibcode:2008A&A...488..151B. ISSN 0004-6361. S2CID 14942349. arXiv:0806.4584 可免费查阅. doi:10.1051/0004-6361:20079255. 
  53. ^ 53.0 53.1 53.2 53.3 53.4 53.5 Bonanos, A. Z.; Lennon, D. J.; Köhlinger, F.; van Loon, J. Th.; Massa, D. L.; Sewilo, M.; Evans, C. J.; Panagia, N.; Babler, B. L.; Block, M.; Bracker, S. Spitzersage-SMC Infrared Photometry of Massive Stars in the Small Magellanic Cloud. The Astronomical Journal. 2010-08-01, 140 (2): 416–429 [2021-07-11]. Bibcode:2010AJ....140..416B. ISSN 0004-6256. S2CID 119290443. arXiv:1004.0949 可免费查阅. doi:10.1088/0004-6256/140/2/416. （原始内容存档于2021-06-06）. 
  54. ^ Crowther, Paul A.; Caballero-Nieves, S. M.; Bostroem, K. A.; Maíz Apellániz, J.; Schneider, F. R. N.; Walborn, N. R.; Angus, C. R.; Brott, I.; Bonanos, A.; De Koter, A.; De Mink, S. E.; Evans, C. J.; Gräfener, G.; Herrero, A.; Howarth, I. D.; Langer, N.; Lennon, D. J.; Puls, J.; Sana, H.; Vink, J. S. The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of He II λ1640 in young star clusters. Monthly Notices of the Royal Astronomical Society. 2016, 458 (1): 624–659. Bibcode:2016MNRAS.458..624C. arXiv:1603.04994 可免费查阅. doi:10.1093/mnras/stw273. 
  55. ^ Van Genderen, A. M. S Doradus variables in the Galaxy and the Magellanic Clouds. Astronomy and Astrophysics. 2001, 366 (2): 508–531. Bibcode:2001A&A...366..508V. doi:10.1051/0004-6361:20000022 可免费查阅. Vizie database entry （页面存档备份，存于互联网档案馆）
  56. ^ Egan, Michael P.; et al. An Infrared Ring Nebula around MSX5C G358.5391+00.1305: The True Nature of Suspected Planetary Nebula Wray 17-96 Determined via Direct Imaging and Spectroscopy. The Astrophysical Journal. 2002, 572 (1): 288–299. Bibcode:2002ApJ...572..288E. doi:10.1086/340222 可免费查阅. 
  57. ^ Tramper, F.; Sana, H.; Fitzsimons, N. E.; De Koter, A.; Kaper, L.; Mahy, L.; Moffat, A. The mass of the very massive binary WR21a. Monthly Notices of the Royal Astronomical Society. 2016, 455 (2): 1275–1281. Bibcode:2016MNRAS.455.1275T. S2CID 44364798. arXiv:1510.03609 可免费查阅. doi:10.1093/mnras/stv2373. 
  58. ^ Najarro, F.; Figer, D. F.; Hillier, D. J.; Geballe, T. R.; Kudritzki, R. P. Metallicity in the Galactic Center: The Quintuplet Cluster. The Astrophysical Journal. 2009, 691 (2): 1816–1827. Bibcode:2009ApJ...691.1816N. S2CID 15473563. arXiv:0809.3185 可免费查阅. doi:10.1088/0004-637X/691/2/1816. 
  59. ^ Oskinova, L. M.; Huenemoerder, D. P.; Hamann, W. -R.; Shenar, T.; Sander, A. A. C.; Ignace, R.; Todt, H.; Hainich, R. On the Binary Nature of Massive Blue Hypergiants: High-resolution X-Ray Spectroscopy Suggests That Cyg OB2 12 is a Colliding Wind Binary. The Astrophysical Journal. 2017, 845 (1): 39. Bibcode:2017ApJ...845...39O. S2CID 119537489. arXiv:1707.04473 可免费查阅. doi:10.3847/1538-4357/aa7e79. 
  60. ^ 60.0 60.1 Laur, Jaan; Kolka, Indrek; Eenmäe, Tõnis; Tuvikene, Taavi; Leedjärv, Laurits. Variability survey of brightest stars in selected OB associations. Astronomy & Astrophysics. 2017, 598: A108. Bibcode:2017A&A...598A.108L. ISSN 0004-6361. S2CID 119076598. arXiv:1611.02452 可免费查阅. doi:10.1051/0004-6361/201629395. 
  61. ^ 61.0 61.1 61.2 61.3 Moffat, A. F. J. On the distance and reddening of the massive H II region NGC 3603. Astronomy and Astrophysics. October 1974, 35: 315. Bibcode:1974A&A....35..315M. ISSN 0004-6361. S2CID 115549707. 
  62. ^ Williams, Peredur. Results from the 2009 campaign on WR 140. Société Royale des Sciences de Liège. 2011, 80: 595–609. Bibcode:2011BSRSL..80..595W. 
  63. ^ 63.0 63.1 Reed, B. Cameron. Catalog of Galactic OB Stars. The Astronomical Journal. 2003, 125 (5): 2531–2533 [2021-07-11]. Bibcode:2003AJ....125.2531R. ISSN 0004-6256. doi:10.1086/374771. （原始内容存档于2021-05-16）. 
  64. ^ 64.0 64.1 64.2 Humphreys, Roberta M.; Davidson, Kris; Hahn, David; Martin, John C.; Weis, Kerstin. Luminous and Variable Stars in M31 and M33 V. The Upper HR Diagram. The Astrophysical Journal. 2017-07-06, 844 (1): 40. Bibcode:2017ApJ...844...40H. S2CID 119357524. arXiv:1707.01916 可免费查阅. doi:10.3847/1538-4357/aa7cef. 
  65. ^ Evans, C. J.; Lennon, D. J.; Smartt, S. J.; Trundle, C. The VLT-FLAMES survey of massive stars: observations centered on the Magellanic Cloud clusters NGC 330, NGC 346, NGC 2004, and the N11 region. Astronomy & Astrophysics. September 2006, 456 (2): 623–638. Bibcode:2006A&A...456..623E. ISSN 0004-6361. S2CID 13160849. arXiv:astro-ph/0606405 可免费查阅. doi:10.1051/0004-6361:20064988. 
  66. ^ Smith, Nathan. A census of the Carina Nebula - I. Cumulative energy input from massive stars. Monthly Notices of the Royal Astronomical Society. 2006, 367 (2): 763–772. Bibcode:2006MNRAS.367..763S. S2CID 14060690. arXiv:astro-ph/0601060 可免费查阅. doi:10.1111/j.1365-2966.2006.10007.x. 
  67. ^ Massey, Philip. A UBVR CCD Survey of the Magellanic Clouds. The Astrophysical Journal Supplement Series. July 2002, 141 (1): 81–122 [2021-07-11]. Bibcode:2002ApJS..141...81M. ISSN 0067-0049. S2CID 119447348. arXiv:astro-ph/0110531 可免费查阅. doi:10.1086/338286. （原始内容存档于2021-07-11）. 
  68. ^ Massey, Philip; Olsen, K. A. G.; Hodge, Paul W.; Jacoby, George H.; McNeill, Reagin T.; Smith, R. C.; Strong, Shay B. A Survey of Local Group Galaxies Currently Forming Stars. II. UBVRI Photometry of Stars in Seven Dwarfs and a Comparison of the Entire Sample. The Astronomical Journal. 2007, 133 (5): 2393–2417. Bibcode:2007AJ....133.2393M. ISSN 0004-6256. S2CID 119456878. arXiv:astro-ph/0702236 可免费查阅. doi:10.1086/513319. 
  69. ^ Lamers, H. J. G. L. M. Proceedings of IAU Colloquium 155, Astrophysical applications of stellar pulsation. Astrophysical Applications of Stellar Pulsation. Astronomical Society of the Pacific Conference Series 83 (Cape Town, South Africa: Astronomical Society of the Pacific). February 6–10, 1995: 176–191. Bibcode:1995ASPC...83..176L.  参数|journal=与模板{{cite conference}}不匹配（建议改用{{cite journal}}或|book-title=） (帮助); |contribution=被忽略 (帮助)
  70. ^ Kastner, J. H.; Buchanan, C. L.; Sargent, B.; Forrest, W. J. SpitzerSpectroscopy of Dusty Disks around B\e] Hypergiants in the Large Magellanic Cloud. The Astrophysical Journal. 2006, 638 (1): L29–L32. Bibcode:2006ApJ...638L..29K. doi:10.1086/500804 可免费查阅. 
  71. ^ Aerts, C.; Lefever, K.; Baglin, A.; Degroote, P.; Oreiro, R.; Vučković, M.; Smolders, K.; Acke, B.; Verhoelst, T.; Desmet, M.; Godart, M.; Noels, A.; Dupret, M.-A.; Auvergne, M.; Baudin, F.; Catala, C.; Michel, E.; Samadi, R. Periodic mass-loss episodes due to an oscillation mode with variable amplitude in the hot supergiant HD 50064. Astronomy and Astrophysics. April 2010, 513: L11. Bibcode:2010A&A...513L..11A. S2CID 41541073. arXiv:1003.5551 可免费查阅. doi:10.1051/0004-6361/201014124. 
  72. ^ Taylor, W. D.; Evans, C. J.; Sana, H.; Walborn, N. R.; De Mink, S. E.; Stroud, V. E.; Alvarez-Candal, A.; Barbá, R. H.; Bestenlehner, J. M.; Bonanos, A. Z.; Brott, I.; Crowther, P. A.; De Koter, A.; Friedrich, K.; Gräfener, G.; Hénault-Brunet, V.; Herrero, A.; Kaper, L.; Langer, N.; Lennon, D. J.; Maíz Apellániz, J.; Markova, N.; Morrell, N.; Monaco, L.; Vink, J. S. The VLT-FLAMES Tarantula Survey II: R139 revealed as a massive binary system. Astronomy & Astrophysics. 2011, 530: L10. Bibcode:2011A&A...530L..10T. S2CID 119214376. arXiv:1103.5387 可免费查阅. doi:10.1051/0004-6361/201116785. 
  73. ^ Ulaczyk, K.; Szymański, M. K.; Udalski, A.; Kubiak, M.; Pietrzyński, G.; Soszyński, I.; Wyrzykowski, Ł.; Poleski, R.; Gieren, W.; Walker, A. R.; Garcia-Varela, A. Variable Stars from the OGLE-III Shallow Survey in the Large Magellanic Cloud. Acta Astronomica. 1 June 2013, 63 (2): 159–179 [2021-07-11]. Bibcode:2013AcA....63..159U. ISSN 0001-5237. S2CID 119228254. arXiv:1306.4802 可免费查阅. （原始内容存档于2022-03-07）. 
  74. ^ 74.0 74.1 Hainich, R.; Pasemann, D.; Todt, H.; Shenar, T.; Sander, A.; Hamann, W. -R. Wolf-Rayet stars in the Small Magellanic Cloud. I. Analysis of the single WN stars. Astronomy & Astrophysics. 2015, 581 (21): 30. Bibcode:2015A&A...581A..21H. S2CID 56230998. arXiv:1507.04000 可免费查阅. doi:10.1051/0004-6361/201526241. 
  75. ^ Rivero González, J. G.; Puls, J.; Najarro, F.; Brott, I. Nitrogen line spectroscopy of O-stars. II. Surface nitrogen abundances for O-stars in the Large Magellanic Cloud. Astronomy & Astrophysics. 2012, 537: A79. Bibcode:2012A&A...537A..79R. ISSN 0004-6361. S2CID 119110554. arXiv:1110.5148 可免费查阅. doi:10.1051/0004-6361/201117790. 
  76. ^ Thompson, Todd A.; Prieto, José L.; Stanek, K. Z.; Kistler, Matthew D.; Beacom, John F.; Kochanek, Christopher S. A New Class of Luminous Transients and a First Census of Their Massive Stellar Progenitors. The Astrophysical Journal. 2009-11-10, 705 (2): 1364–1384. Bibcode:2009ApJ...705.1364T. ISSN 0004-637X. S2CID 17581579. arXiv:0809.0510 可免费查阅. doi:10.1088/0004-637X/705/2/1364. hdl:1811/48176. 
  77. ^ Sander, A. A. C.; Hamann, W.-R.; Todt, H.; Hainich, R.; Shenar, T.; Ramachandran, V.; Oskinova, L. M. The Galactic WC and WO stars. Astronomy & Astrophysics. 2019, 621: A92. Bibcode:2019A&A...621A..92S. S2CID 67754788. arXiv:1807.04293 可免费查阅. doi:10.1051/0004-6361/201833712. 
  78. ^ 78.0 78.1 Rauw; et al. The spectrum of the very massive binary system WR 20a (WN6ha + WN6ha): Fundamental parameters and wind interactions (PDF). Astronomy & Astrophysics. 4 March 2005, 432 (3): 985–998 [2021-07-11]. Bibcode:2005A&A...432..985R. doi:10.1051/0004-6361:20042136 可免费查阅. （原始内容存档 (PDF)于2020-08-03）. 
  79. ^ 79.0 79.1 Peeples, Molly S.; Bonanos, A. Z.; DePoy, D. L.; Stanek, K. Z.; Pepper, J.; Pogge, Richard W.; Pinsonneault, M. H.; Sellgren, K. The Nature of the Variable Galactic Center Source GCIRS 16SW Revisited: A Massive Eclipsing Binary. The Astrophysical Journal. 2007-01-01, 654 (1): L61–L64 [2021-07-11]. Bibcode:2007ApJ...654L..61P. ISSN 0004-637X. S2CID 14242573. arXiv:astro-ph/0610212 可免费查阅. doi:10.1086/510720. （原始内容存档于2021-01-21）. 
  80. ^ Morrell, N. I.; Barbá, R. H.; Niemela, V. S.; Corti, M. A.; Albacete Colombo, J. F.; Rauw, G.; Corcoran, M.; Morel, T.; Bertrand, J.-F.; Moffat, A. F. J.; St-Louis, N. Optical spectroscopy of X-Mega targets - II. The massive double-lined O-type binary HD 93205 (PDF). Monthly Notices of the Royal Astronomical Society. 2001, 326 (1): 85–94 [2021-07-11]. Bibcode:2001MNRAS.326...85M. S2CID 16221731. arXiv:astro-ph/0105014 可免费查阅. doi:10.1046/j.1365-8711.2001.04500.x. （原始内容存档 (PDF)于2017-08-18）. 
  81. ^ 81.0 81.1 Neugent, Kathryn F.; Massey, Philip. The Wolf-Rayet Content of M33. The Astrophysical Journal. 2011-06-01, 733 (2): 123 [2021-07-11]. Bibcode:2011ApJ...733..123N. ISSN 0004-637X. S2CID 118507918. arXiv:1103.5549 可免费查阅. doi:10.1088/0004-637X/733/2/123. （原始内容存档于2021-06-06）. 
  82. ^ Walborn, N. R.; Sana, H.; Simón-Díaz, S.; Maíz Apellániz, J.; Taylor, W. D.; Evans, C. J.; Markova, N.; Lennon, D. J.; de Koter, A. The VLT-FLAMES Tarantula Survey. XIV. The O-type stellar content of 30 Doradus. Astronomy & Astrophysics. 2014, 564 (40): 35. Bibcode:2014A&A...564A..40W. S2CID 119302111. arXiv:1402.6969 可免费查阅. doi:10.1051/0004-6361/201323082. 
  83. ^ Rauw, G.; Vreux, J.-M.; Stevens, I. R.; Gosset, E.; Sana, H.; Jamar, C.; Mason, K. O. Phase-resolved X-ray and optical spectroscopy of the massive binary HD 93403. Astronomy and Astrophysics. 2002, 388 (2): 552. Bibcode:2002A&A...388..552R. doi:10.1051/0004-6361:20020523 可免费查阅. 
  84. ^ Crowther, P. A.; Hadfield, L. J.; Clark, J. S.; Negueruela, I.; Vacca, W. D. A census of the Wolf-Rayet content in Westerlund 1 from near-infrared imaging and spectroscopy. Monthly Notices of the Royal Astronomical Society. 2006-11-01, 372 (3): 1407–1424. Bibcode:2006MNRAS.372.1407C. ISSN 0035-8711. S2CID 10505573. arXiv:astro-ph/0608356 可免费查阅. doi:10.1111/j.1365-2966.2006.10952.x. 
  85. ^ Clark, J. S.; Muno, M. P.; Negueruela, I.; Dougherty, S. M.; Crowther, P. A.; Goodwin, S. P.; de Grijs, R. Unveiling the X-ray point source population of the Young Massive Cluster Westerlund 1. Astronomy & Astrophysics. 2008, 477 (1): 147–163. Bibcode:2008A&A...477..147C. ISSN 0004-6361. doi:10.1051/0004-6361:20077186 可免费查阅. 
  86. ^ 86.0 86.1 86.2 86.3 Repolust, T.; Puls, J.; Herrero, A. Stellar and wind parameters of Galactic O-stars. The influence of line-blocking/blanketing. Astronomy and Astrophysics. 2004, 415: 349. Bibcode:2004A&A...415..349R. doi:10.1051/0004-6361:20034594 可免费查阅. 
  87. ^ Neugent, Kathryn F.; Massey, Philip; Morrell, Nidia. The Discovery of a Rare Wo-Type Wolf–Rayet Star in the Large Magellanic Cloud. The Astronomical Journal. 2012-12-01, 144 (6): 162 [2021-07-11]. Bibcode:2012AJ....144..162N. ISSN 0004-6256. S2CID 118628394. arXiv:1210.0062 可免费查阅. doi:10.1088/0004-6256/144/6/162. （原始内容存档于2021-10-26）. 
  88. ^ Clark, J. S.; Najarro, F.; Negueruela, I.; Ritchie, B. W.; Urbaneja, M. A.; Howarth, I. D. On the nature of the galactic early-B hypergiants. Astronomy & Astrophysics. 2012, 541: A145. Bibcode:2012A&A...541A.145C. ISSN 0004-6361. S2CID 11978733. arXiv:1202.3991 可免费查阅. doi:10.1051/0004-6361/201117472. 
  89. ^ Kozok, J. R., Photometric observations of emission B-stars in the southern Milky Way, Astronomy and Astrophysics Supplement Series, September 1985, 61: 387–405, Bibcode:1985A&AS...61..387K 
  90. ^ 90.0 90.1 Bouret, J. -C.; Hillier, D. J.; Lanz, T.; Fullerton, A. W. Properties of Galactic early-type O-supergiants: A combined FUV-UV and optical analysis. Astronomy & Astrophysics. 2012, 544: A67. Bibcode:2012A&A...544A..67B. S2CID 119280104. arXiv:1205.3075v1 可免费查阅. doi:10.1051/0004-6361/201118594. 
  91. ^ Rivet, J-P; Siciak, A.; de Almeida, E. S. G.; Vakili, F.; Domiciano de Souza, A.; Fouché, M.; Lai, O.; Vernet, D.; Kaiser, R.; Guerin, W. Intensity interferometry of P Cygni in the H α emission line: Towards distance calibration of LBV supergiant stars. Monthly Notices of the Royal Astronomical Society. 2020, 494: 218–227. Bibcode:2020MNRAS.494..218R. S2CID 204788654. arXiv:1910.08366 可免费查阅. doi:10.1093/mnras/staa588. 
  92. ^ Skinner, Stephen L.; Zhekov, Svetozar A.; Güdel, Manuel; Schmutz, Werner; Sokal, Kimberly R. New X-Ray Detections of WNL Stars. The Astronomical Journal. 2012-05-01, 143 (5): 116 [2021-07-11]. Bibcode:2012AJ....143..116S. ISSN 0004-6256. S2CID 119281411. arXiv:1203.5098 可免费查阅. doi:10.1088/0004-6256/143/5/116. （原始内容存档于2021-06-05）. 
  93. ^ 93.0 93.1 93.2 Searle, S. C.; Prinja, R. K.; Massa, D.; Ryans, R. Quantitative studies of the optical and UV spectra of Galactic early B supergiants. I. Fundamental parameters. Astronomy and Astrophysics. 2008, 481 (3): 777–97. Bibcode:2008A&A...481..777S. S2CID 1552752. arXiv:0801.4289 可免费查阅. doi:10.1051/0004-6361:20077125. 
  94. ^ Mehner, Andrea; Davidson, Kris; Ferland, Gary J.; Humphreys, Roberta M. High-excitation Emission Lines near Eta Carinae, and Its Likely Companion Star. The Astrophysical Journal. 2010, 710 (1): 729–742. Bibcode:2010ApJ...710..729M. S2CID 5032987. arXiv:0912.1067 可免费查阅. doi:10.1088/0004-637X/710/1/729. 
  95. ^ 95.0 95.1 95.2 95.3 95.4 95.5 Hohle, M. M.; Neuhäuser, R.; Schutz, B. F., Masses and luminosities of O- and B-type stars and red supergiants, Astronomische Nachrichten, April 2010, 331 (4): 349, Bibcode:2010AN....331..349H, S2CID 111387483, arXiv:1003.2335 可免费查阅, doi:10.1002/asna.200911355 
  96. ^ 96.0 96.1 North, J. R.; Tuthill, P. G.; Tango, W. J.; Davis, J. γ2 Velorum: orbital solution and fundamental parameter determination with SUSI. Monthly Notices of the Royal Astronomical Society. 2007-05-01, 377 (1): 415–424 [2021-07-11]. Bibcode:2007MNRAS.377..415N. ISSN 0035-8711. S2CID 16425744. arXiv:astro-ph/0702375 可免费查阅. doi:10.1111/j.1365-2966.2007.11608.x. （原始内容存档于2022-02-02）. 
  97. ^ Hummel, C. A.; Rivinius, Th.; Nieva, M.-F.; Stahl, O.; van Belle, G.; Zavala, R. T. Dynamical mass of the O-type supergiant in ζ Orionis A. Astronomy & Astrophysics. 2013, 554: A52. Bibcode:2013A&A...554A..52H. ISSN 0004-6361. S2CID 53645495. arXiv:1306.0330 可免费查阅. doi:10.1051/0004-6361/201321434. 
  98. ^ Nugis, T.; Lamers, H. J. G. L. M. Mass-loss rates of Wolf-Rayet stars as a function of stellar parameters. Astronomy and Astrophysics. 2000, 360: 227. Bibcode:2000A&A...360..227N. 
  99. ^ Crowther, P. A.; Lennon, D. J.; Walborn, N. R., Physical parameters and wind properties of galactic early B supergiants, Astronomy and Astrophysics, January 2006, 446 (1): 279–293, Bibcode:2006A&A...446..279C, S2CID 18815761, arXiv:astro-ph/0509436 可免费查阅, doi:10.1051/0004-6361:20053685 
  100. ^ Simón-Díaz, S.; Herrero, A.; Esteban, C.; Najarro, F. Detailed spectroscopic analysis of the Trapezium cluster stars inside the Orion nebula: Rotational velocities, stellar parameters, and oxygen abundances. Astronomy & Astrophysics. 2006, 448 (1): 351–366. Bibcode:2006A&A...448..351S. ISSN 0004-6361. S2CID 16445304. arXiv:astro-ph/0510288 可免费查阅. doi:10.1051/0004-6361:20053066. 
  101. ^ Shenar, T.; Oskinova, L.; Hamann, W.-R.; Corcoran, M. F.; Moffat, A. F. J.; Pablo, H.; Richardson, N. D.; Waldron, W. L.; Huenemoerder, D. P.; Maíz Apellániz, J.; Nichols, J. S.; Todt, H.; Nazé, Y.; Hoffman, J. L.; Pollock, A. M. T.; Negueruela, I. A Coordinated X-Ray and Optical Campaign of the Nearest Massive Eclipsing Binary, δ Orionis Aa. IV. A Multiwavelength, Non-LTE Spectroscopic Analysis. Astrophysical Journal. 2015, 809 (2): 135. Bibcode:2015ApJ...809..135S. S2CID 14909574. arXiv:1503.03476 可免费查阅. doi:10.1088/0004-637X/809/2/135. hdl:10045/59172. 
  102. ^ Tokovinin, A. A. MSC - a catalogue of physical multiple stars. Astronomy and Astrophysics Supplement Series. 1997, 124: 75–84. Bibcode:1997A&AS..124...75T. doi:10.1051/aas:1997181 可免费查阅. 
  103. ^ Murdin, P.; Penston, M. V. The Lambda Orionis association. Monthly Notices of the Royal Astronomical Society. 1977-12-01, 181 (4): 657–665 [2021-07-11]. Bibcode:1977MNRAS.181..657M. ISSN 0035-8711. doi:10.1093/mnras/181.4.657 可免费查阅. （原始内容存档于2021-10-29）. 
  104. ^ 104.0 104.1 104.2 Hoffleit, Dorrit; Jaschek, Carlos. The Bright star catalogue 5th Revised. New Haven, Conn.: Yale University Observatory. 1991. Bibcode:1991bsc..book.....H. 
  105. ^ Moravveji, Ehsan; Guinan, Edward F.; Shultz, Matt; Williamson, Michael H.; Moya, Andres. Asteroseismology of the Nearby SN-II Progenitor: Rigel. I. Themosthigh-Precision Photometry and Radial Velocity Monitoring. The Astrophysical Journal. 2012-03-10, 747 (2): 108 [2021-07-11]. Bibcode:2012ApJ...747..108M. ISSN 0004-637X. S2CID 425831. arXiv:1201.0843 可免费查阅. doi:10.1088/0004-637X/747/2/108. （原始内容存档于2021-03-24）. 
  106. ^ Hillenbrand, Lynne A. On the Stellar Population and Star-Forming History of the Orion Nebula Cluster. Astronomical Journal. 1997, 113: 1733. Bibcode:1997AJ....113.1733H. doi:10.1086/118389. 
  107. ^ Aldoretta, E. J.; Caballero-Nieves, S. M.; Gies, D. R.; Nelan, E. P.; Wallace, D. J.; Hartkopf, W. I.; Henry, T. J.; Jao, W.-C.; Maíz Apellániz, J.; Mason, B. D.; Moffat, A. F. J.; Norris, R. P.; Richardson, N. D.; Williams, S. J. The Multiplicity of Massive Stars: A High Angular Resolution Survey with the Guidance Sensor. The Astronomical Journal. 2015, 149 (1): 26. Bibcode:2015AJ....149...26A. S2CID 58911264. arXiv:1410.0021 可免费查阅. doi:10.1088/0004-6256/149/1/26. 
  108. ^ 108.0 108.1 Marchenko, Sergey V.; Rauw, Gregor; Antokhina, Eleonora A.; Antokhin, Igor I.; Ballereau, Dominique; Chauville, Jacques; Corcoran, Michael F.; Costero, Rafael; Echevarria, Juan; Eversberg, Thomas; Gayley, Ken G.; Koenigsberger, Gloria; Miroshnichenko, Anatoly S.; Moffat, Anthony F. J.; Morrell, Nidia I.; Morrison, Nancy D.; Mulliss, Christopher L.; Pittard, Julian M.; Stevens, Ian R.; Vreux, Jean-Marie; Zorec, Jean. Coordinated monitoring of the eccentric O-star binary Iota Orionis: Optical spectroscopy and photometry. Monthly Notices of the Royal Astronomical Society. 2000, 317 (2): 333. Bibcode:2000MNRAS.317..333M. doi:10.1046/j.1365-8711.2000.03542.x 可免费查阅. 
  109. ^ 109.0 109.1 109.2 Nicolet, B., Photoelectric photometric Catalogue of homogeneous measurements in the UBV System, Astronomy and Astrophysics Supplement Series, 1978, 34: 1–49, Bibcode:1978A&AS...34....1N 
  110. ^ Underhill, A. B.; Divan, L.; Prevot-Burnichon, M.-L.; Doazan, V. Effective temperatures, angular diameters, distances and linear radii for 160 O and B stars. Monthly Notices of the Royal Astronomical Society. 1979, 189 (3): 601–05. Bibcode:1979MNRAS.189..601U. doi:10.1093/mnras/189.3.601 可免费查阅. 
  111. ^ Nieva, M.-F. Temperature, gravity, and bolometric correction scales for non-supergiant OB stars. Astronomy & Astrophysics. 2013, 550: A26. Bibcode:2013A&A...550A..26N. ISSN 0004-6361. S2CID 119275940. arXiv:1212.0928 可免费查阅. doi:10.1051/0004-6361/201219677. 
  112. ^ Tanrıverdi, Taner. Elemental abundances of the supergiant stars σ Cygnus and η Leonis. New Astronomy. 2013, 25: 50. Bibcode:2013NewA...25...50T. S2CID 118525375. arXiv:1512.04557 可免费查阅. doi:10.1016/j.newast.2013.03.013. 
  113. ^ Firnstein, M.; Przybilla, N. Quantitative spectroscopy of Galactic BA-type supergiants. I. Atmospheric parameters. Astronomy & Astrophysics. 2012, 543: A80. Bibcode:2012A&A...543A..80F. S2CID 54725386. arXiv:1207.0308 可免费查阅. doi:10.1051/0004-6361/201219034. 
  114. ^ Martins, F.; Schaerer, D.; Hillier, D. J.; Meynadier, F.; Heydari-Malayeri, M.; Walborn, N. R. O stars with weak winds: the Galactic case. Astronomy & Astrophysics. 2005, 441 (2): 735–762. Bibcode:2005A&A...441..735M. ISSN 0004-6361. S2CID 11547293. arXiv:astro-ph/0507278 可免费查阅. doi:10.1051/0004-6361:20052927. 
  115. ^ 115.0 115.1 115.2 Simón-Díaz, S.; Caballero, J. A.; Lorenzo, J.; Maíz Apellániz, J.; Schneider, F. R. N.; Negueruela, I.; Barbá, R. H.; Dorda, R.; Marco, A.; Montes, D.; Pellerin, A.; Sanchez-Bermudez, J.; Sódor, Á.; Sota, A. Orbital and Physical Properties of the σ Ori Aa, Ab, B Triple System. The Astrophysical Journal. 2015, 799 (2): 169. Bibcode:2015ApJ...799..169S. S2CID 118500350. arXiv:1412.3469 可免费查阅. doi:10.1088/0004-637X/799/2/169. 
  116. ^ 116.0 116.1 116.2 Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog. The Astronomical Journal. 2001, 122 (6): 3466. Bibcode:2001AJ....122.3466M. doi:10.1086/323920 可免费查阅. 
  117. ^ Pecaut, Mark J.; Mamajek, Eric E.; Bubar, Eric J. A Revised Age for Upper Scorpius and the Star Formation History Among the F-Type Members of the Scorpius-Centaurus Ob Association. The Astrophysical Journal. 2012-02-20, 746 (2): 154 [2021-07-11]. Bibcode:2012ApJ...746..154P. ISSN 0004-637X. S2CID 118461108. arXiv:1112.1695 可免费查阅. doi:10.1088/0004-637X/746/2/154. （原始内容存档于2021-02-25）. 
  118. ^ Gutierrez-Moreno, Adelina; Moreno, Hugo. A Photometric Investigation of the SCORPlO-CENTAURUS Association. The Astrophysical Journal Supplement Series. 1968-06-01, 15: 459 [2021-07-11]. Bibcode:1968ApJS...15..459G. ISSN 0067-0049. doi:10.1086/190168. （原始内容存档于2019-03-25）. 
  119. ^ Lutz, T. E.; Lutz, J. H., Spectral classification and UBV photometry of bright visual double stars, Astronomical Journal, June 1977, 82: 431–434, Bibcode:1977AJ.....82..431L, doi:10.1086/112066 
  120. ^ 120.0 120.1 120.2 Johnson, H. L.; et al, UBVRIJKL photometry of the bright stars, Communications of the Lunar and Planetary Laboratory, 1966, 4 (99): 99, Bibcode:1966CoLPL...4...99J 
  121. ^ Hubrig, S.; et al, Discovery of magnetic fields in the βCephei star ξ1 CMa and in several slowly pulsating B stars*, Monthly Notices of the Royal Astronomical Society: Letters, June 2006, 369 (1): L61–L65, Bibcode:2006MNRAS.369L..61H, S2CID 18201908, arXiv:astro-ph/0604283 可免费查阅, doi:10.1111/j.1745-3933.2006.00175.x 
  122. ^ Cousins, A. W. J., UBV Photometry of Some Very Bright Stars, Monthly Notes of the Astronomical Society of Southern Africa, 1972, 31: 69, Bibcode:1972MNSSA..31...69C 
  123. ^ Nieva, María-Fernanda; Przybilla, Norbert. Fundamental properties of nearby single early B-type stars. Astronomy & Astrophysics. 2014, 566: A7. Bibcode:2014A&A...566A...7N. S2CID 119227033. arXiv:1412.1418 可免费查阅. doi:10.1051/0004-6361/201423373. 
  124. ^ Nicolet, B. Catalogue of homogeneous data in the UBV photoelectric photometric system. Astronomy and Astrophysics Supplement Series. October 1978, 34: 1–49. Bibcode:1978A&AS...34....1N. 
  125. ^ Pillitteri, I.; Fossati, L.; Castro Rodriguez, N.; Oskinova, L.; Wolk, S. J. Detection of magnetic field in the B2 star ρ Ophiuchi A with ESO FORS2. Astronomy & Astrophysics. 2018, 610: L3. Bibcode:2018A&A...610L...3P. ISSN 0004-6361. S2CID 119395824. arXiv:1712.00728 可免费查阅. doi:10.1051/0004-6361/201732078. 
  126. ^ 126.0 126.1 126.2 126.3 126.4 126.5 126.6 Anderson, E.; Francis, Ch. XHIP: An extended hipparcos compilation. Astronomy Letters. 2012, 38 (5): 331. Bibcode:2012AstL...38..331A. S2CID 119257644. arXiv:1108.4971 可免费查阅. doi:10.1134/S1063773712050015.  Vizier catalog entry （页面存档备份，存于互联网档案馆）
  127. ^ Kudritzki, R. P.; Reimers, D. On the absolute scale of mass-loss in red giants. II. Circumstellar absorption lines in the spectrum of alpha Sco B and mass-loss of alpha Sco A. Astronomy and Astrophysics. 1978, 70: 227. Bibcode:1978A&A....70..227K. 
  128. ^ Jerzykiewicz, M.; Molenda-Zakowicz, J., Empirical Luminosities and Radii of Early-Type Stars after Hipparcos, Acta Astronomica, September 2000, 50: 369–380, Bibcode:2000AcA....50..369J 
  129. ^ Harmanec, P. Physical Properties and Evolutionary Stage of Be Stars. The be Phenomenon in Early-Type Stars. 2000, 214: 13. Bibcode:2000ASPC..214...13H. 
  130. ^ Fernie, J. D., New UBVRI photometry for 900 supergiants, Astrophysical Journal Supplement Series, May 1983, 52: 7–22, Bibcode:1983ApJS...52....7F, doi:10.1086/190856. 
  131. ^ Feinstein, A.; Marraco, H. G., The photometric behavior of Be Stars, Astronomical Journal, November 1979, 84: 1713–1725, Bibcode:1979AJ.....84.1713F, doi:10.1086/112600. 
  132. ^ McDonald, I.; et al, Fundamental Parameters and Infrared Excesses of Hipparcos Stars, Monthly Notices of the Royal Astronomical Society, 2012, 427 (1): 343–57, Bibcode:2012MNRAS.427..343M, S2CID 118665352, arXiv:1208.2037 可免费查阅, doi:10.1111/j.1365-2966.2012.21873.x. 
  133. ^ Mermilliod, J.-C., Compilation of Eggen's UBV data, transformed to UBV (unpublished), Catalogue of Eggen's UBV Data (SIMBAD), 1986, Bibcode:1986EgUBV........0M. 
  134. ^ North, P. Do SI stars undergo any rotational braking?. Astronomy and Astrophysics. 1998, 334: 181–87. Bibcode:1998A&A...334..181N. arXiv:astro-ph/9802286 可免费查阅. 
  135. ^ Fang, M.; et al, Young stars in ɛ Chamaleontis and their disks: disk evolution in sparse associations (PDF), Astronomy & Astrophysics, January 2013, 549: 17, Bibcode:2013A&A...549A..15F, S2CID 118332644, arXiv:1209.5832 可免费查阅, doi:10.1051/0004-6361/201118528, A15. 
  136. ^ Zorec, J.; Royer, F. Rotational velocities of A-type stars. Astronomy & Astrophysics. 2012, 537: A120. Bibcode:2012A&A...537A.120Z. S2CID 55586789. arXiv:1201.2052 可免费查阅. doi:10.1051/0004-6361/201117691.  Vizier catalog entry （页面存档备份，存于互联网档案馆）
  137. ^ Corben, P. M.; Stoy, R. H., Photoelectric Magnitudes and Colours for Bright Southern Stars, Monthly Notes of the Astronomical Society of Southern Africa, 1968, 27: 11, Bibcode:1968MNSSA..27...11C. 
  138. ^ Silaj, J.; et al, The Hα Profiles of Be Shell Stars, The Astrophysical Journal, November 2014, 795 (1): 12, Bibcode:2014ApJ...795...82S, doi:10.1088/0004-637X/795/1/82, 82. 
  139. ^ International Astronomical Union 2015 RESOLUTION (PDF), International Astronomical Union, 13 August 2015 [2021-07-11], （原始内容存档 (PDF)于2016-01-28） 
  140. ^ Luzum, Brian; Capitaine, Nicole; Fienga, Agnès; Folkner, William; Fukushima, Toshio; Hilton, James; Hohenkerk, Catherine; Krasinsky, George; Petit, Gérard; Pitjeva, Elena; Soffel, Michael. The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy. Celestial Mechanics and Dynamical Astronomy. August 2011, 110 (4): 293–304. Bibcode:2011CeMDA.110..293L. ISSN 0923-2958. doi:10.1007/s10569-011-9352-4 可免费查阅. 
  141. ^ Bessell, M.S.; Castelli, F.; Plez, B. Model atmospheres broad-band colors, bolometric corrections and temperature calibrations for O–M stars. Astronomy and Astrophysics. 1998, 333: 231–250. Bibcode:1998A&A...333..231B. 

外部連結

[编辑]
检索自“https://zh.wikipedia.org/zhwiki/w/index.php?title=恆星光度列表&oldid=74180763”