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Coordinates: Sky map 11h 26m 08.5689s, +43° 35′ 09.696″
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{{short description|Galaxy in the constellation Ursa Major}}
{{short description|Galaxy in the constellation Ursa Major}}
{{Sky|11|26|08.5689|+|43|35|09.696}}
{{Infobox galaxy
{{Infobox galaxy
| name = [[New General Catalogue|NGC]] 3675
| name = [[New General Catalogue|NGC]] 3675
| image = NGC3675 spiral galaxy in Schulman telescope.jpg
| image = NGC3675 spiral galaxy in Schulman telescope.jpg
⚫
| caption = NGC 3675 in Schulman telescope
| image_size = 250px
⚫
| caption = NGC 3675 in Schulman telescope
| credit =
| credit =
| epoch = [[J2000]]
| epoch = [[J2000]]
| type = SA(s)b <ref name="ned">{{cite web
| type = SA(s)b <ref name="ned">{{cite web
| title=NASA/IPAC Extragalactic Database
| title=NASA/IPAC Extragalactic Database
| work=Results for NGC 3675
| work=Results for object NGC 3675
| url=http://ned.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=NGC+3675
| url=https://ned.ipac.caltech.edu/byname?objname=ngc+3675
| access-date=2016-01-18 }}</ref>
| access-date=2016-01-18 }}</ref>
| ra = {{RA|11|26|08.6}}<ref name="ned" />
| ra = {{RA|11|26|08.5689}}<ref name="ned" />
| dec = {{DEC|43|35|09}}<ref name="ned" />
| dec = {{DEC|+43|35|09.696}}<ref name="ned" />
| dist_ly = [[1 E23 m|53]] ± 10 [[light-year|Mly]] (16.2 ± 3.0 [[parsec|Mpc]])<ref name="ned" />
| dist_ly = [[1 E23 m|53]] ± 10 [[light-year|Mly]] (16.2 ± 3.0 [[parsec|Mpc]])<ref name="ned" />
| z = 770 ± 1 [[kilometer|km]]/[[second|s]]<ref name="ned" />
| z = 0.002568<ref name="ned" />
| h_radial_v = 770 ± 1 km/s<ref name="ned" />
| appmag_v = 10.0
| appmag_v = 10.0
| size = ~{{convert|32.41|kpc|ly|abbr=on|lk=on|order=flip}} (estimated)<ref name ="ned" />
| size_v = 5.9{{prime}} × 3.1{{prime}}<ref name="ned" />
| size_v = 5.9{{prime}} × 3.1{{prime}}<ref name="ned" />
| constellation name = [[Ursa Major]]
| constellation name = [[Ursa Major]]
| notes =
| notes =
| names = [[Uppsala General Catalogue|UGC]] 6439, [[Morphological Catalogue of Galaxies|MCG]] +07-24-004, [[Principal Galaxies Catalogue|PGC]] 35164<ref name="ned" />
| names = {{odlist | UGC= 6439 | MCG= +07-24-004 | PGC= 35164 | CGCG= 214-005 | IRAS= 11234+4351}}<ref name="ned" />
}}
}}
'''NGC 3675''' is a [[spiral galaxy]] located in the constellation [[Ursa Major]]. It is located at a distance of circa 50 million [[light year]]s from Earth, which, given its apparent dimensions, means that NGC 3675 is about 100,000 light years across. It was discovered by [[William Herschel]] in 1788.
'''NGC 3675''' is a [[spiral galaxy]] located in the constellation [[Ursa Major]]. It is located at a distance of about 50 million [[light year]]s from Earth, which, given its apparent dimensions, means that NGC 3675 is about 100,000 light years across. It was discovered by [[Germany|German-British]] astronomer [[William Herschel]] on 14 January 1788.<ref name="selig">{{cite web | url = https://cseligman.com/text/atlas/ngc36a.htm#3675 | title = New General Catalogue Objects: NGC{{nbsp}}3675 | last = Seligman | first = Courtney | website = Celestial Atlas | access-date = 5 December 2024}}</ref> NGC 3675 belongs to the [[Ursa Major Cluster]], part of the [[Virgo Supercluster]].<ref>{{cite web|title=The Ursa Major Groups | url=http://www.atlasoftheuniverse.com/galgrps/uma.html | website=www.atlasoftheuniverse.com}}</ref>


It hosts a [[low-ionization nuclear emission-line region]] (LINER).<ref>{{cite journal|last1=McKernan|first1=B.|last2=Ford|first2=K. E. S.|last3=Reynolds|first3=C. S.|title=Black hole mass, host galaxy classification and AGN activity|journal=Monthly Notices of the Royal Astronomical Society|date=20 July 2010|volume=407|issue=4|pages=2399–2410|doi=10.1111/j.1365-2966.2010.17068.x|arxiv = 1005.4907 |bibcode = 2010MNRAS.407.2399M |s2cid=118679872}}</ref> In the nucleus there is a [[supermassive black hole]] with an estimated mass of 10-39 million {{solar mass|link=y}}, based on the intrinsic velocity dispersion as measured by the [[Hubble Space Telescope]].<ref>{{cite journal|last1=Beifiori|first1=A.|last2=Sarzi|first2=M.|last3=Corsini|first3=E. M.|last4=Bontà|first4=E. Dalla|last5=Pizzella|first5=A.|last6=Coccato|first6=L.|last7=Bertola|first7=F.|title=Upper Limits on the Masses of 105 Supermassive Black Holes from Hubble Space Telescope/Space Telescope Imaging Spectrograph Archival Data|journal=The Astrophysical Journal|date=10 February 2009|volume=692|issue=1|pages=856–868|doi=10.1088/0004-637X/692/1/856|arxiv = 0809.5103 |bibcode = 2009ApJ...692..856B |s2cid=54903233}}</ref> Although the galaxy was reported to have a strong [[barred spiral galaxy|bar]] visible in [[infrared]] images, there has been no indication of a bar in further observations.<ref>{{cite journal|last1=Möllenhoff|first1=C.|last2=Heidt|first2=J.|title=Surface photometry of spiral galaxies in NIR:Structural parameters of disks and bulges|journal=Astronomy & Astrophysics|date=15 March 2001|volume=368|issue=1|pages=16–37|doi=10.1051/0004-6361:20000335|url=https://www.aanda.org/articles/aa/full/2001/10/aa10227/aa10227.html|bibcode = 2001A&A...368...16M |doi-access=free}}</ref> Its [[galaxy disk|spiral disk]] is of type III and there is a dust structure which is more prominent to the east.<ref>{{cite journal|last1=Gutiérrez|first1=Leonel|last2=Erwin|first2=Peter|last3=Aladro|first3=Rebeca|last4=Beckman|first4=John E.|title=The Outer Disks of Early-type Galaxies. II. Surface-brightness Profiles of Unbarred Galaxies and Trends with Hubble Type|journal=The Astronomical Journal|date=1 November 2011|volume=142|issue=5|pages=145|doi=10.1088/0004-6256/142/5/145|arxiv = 1108.3662 |bibcode = 2011AJ....142..145G |s2cid=118386795}}</ref> The galaxy features two ring structures, with diameter 1.62 and 2.42 arcminutes.<ref>{{cite journal|last1=Comerón|first1=S.|last2=Salo|first2=H.|last3=Laurikainen|first3=E.|last4=Knapen|first4=J. H.|last5=Buta|first5=R. J.|last6=Herrera-Endoqui|first6=M.|last7=Laine|first7=J.|last8=Holwerda|first8=B. W.|last9=Sheth|first9=K.|last10=Regan|first10=M. W.|last11=Hinz|first11=J. L.|last12=Muñoz-Mateos|first12=J. C.|last13=Gil de Paz|first13=A.|last14=Menéndez-Delmestre|first14=K.|last15=Seibert|first15=M.|last16=Mizusawa|first16=T.|last17=Kim|first17=T.|last18=Erroz-Ferrer|first18=S.|last19=Gadotti|first19=D. A.|last20=Athanassoula|first20=E.|author20-link=Lia Athanassoula|last21=Bosma|first21=A.|last22=Ho|first22=L. C.|title=ARRAKIS: atlas of resonance rings as known in the S4G|journal=Astronomy & Astrophysics|date=19 February 2014|volume=562|pages=A121|doi=10.1051/0004-6361/201321633|arxiv = 1312.0866 |bibcode = 2014A&A...562A.121C |s2cid=119295831}}</ref> The [[Spiral galaxy#Spiral_arms_Spiral_arms|spiral arm]]s are tightly wound and form an inner pseudoring and they continue for one revolution outside the ring. The outer arms are very patchy and filamentary.<ref>{{cite journal|last1=Eskridge|first1=Paul B.|last2=Frogel|first2=Jay A.|last3=Pogge|first3=Richard W.|last4=Quillen|first4=Alice C.|last5=Berlind|first5=Andreas A.|last6=Davies|first6=Roger L.|last7=DePoy|first7=D. L.|last8=Gilbert|first8=Karoline M.|last9=Houdashelt|first9=Mark L.|last10=Kuchinski|first10=Leslie E.|last11=Ramirez|first11=Solange V.|last12=Sellgren|first12=K.|last13=Stutz|first13=Amelia|last14=Terndrup|first14=Donald M.|last15=Tiede|first15=Glenn P.|title=Near-Infrared and Optical Morphology of Spiral Galaxies|journal=The Astrophysical Journal Supplement Series|date=November 2002|volume=143|issue=1|pages=73–111|doi=10.1086/342340|arxiv = astro-ph/0206320 |bibcode = 2002ApJS..143...73E |s2cid=15491635}}</ref>
It hosts a [[low-ionization nuclear emission-line region]] (LINER).<ref>{{cite journal|last1=McKernan|first1=B.|last2=Ford|first2=K. E. S.|last3=Reynolds|first3=C. S.|title=Black hole mass, host galaxy classification and AGN activity|journal=Monthly Notices of the Royal Astronomical Society|date=20 July 2010|volume=407|issue=4|pages=2399–2410|doi=10.1111/j.1365-2966.2010.17068.x|doi-access=free |arxiv = 1005.4907 |bibcode = 2010MNRAS.407.2399M |s2cid=118679872}}</ref> In the nucleus there is a [[supermassive black hole]] with an estimated mass of 10-39 million {{solar mass|link=y}}, based on the intrinsic velocity dispersion as measured by the [[Hubble Space Telescope]].<ref>{{cite journal|last1=Beifiori|first1=A.|last2=Sarzi|first2=M.|last3=Corsini|first3=E. M.|last4=Bontà|first4=E. Dalla|last5=Pizzella|first5=A.|last6=Coccato|first6=L.|last7=Bertola|first7=F.|title=Upper Limits on the Masses of 105 Supermassive Black Holes from Hubble Space Telescope/Space Telescope Imaging Spectrograph Archival Data|journal=The Astrophysical Journal|date=10 February 2009|volume=692|issue=1|pages=856–868|doi=10.1088/0004-637X/692/1/856|arxiv = 0809.5103 |bibcode = 2009ApJ...692..856B |s2cid=54903233}}</ref> Although the galaxy was reported to have a strong [[barred spiral galaxy|bar]] visible in [[infrared]] images, there has been no indication of a bar in further observations.<ref>{{cite journal|last1=Möllenhoff|first1=C.|last2=Heidt|first2=J.|title=Surface photometry of spiral galaxies in NIR:Structural parameters of disks and bulges|journal=Astronomy & Astrophysics|date=15 March 2001|volume=368|issue=1|pages=16–37|doi=10.1051/0004-6361:20000335|url=https://www.aanda.org/articles/aa/full/2001/10/aa10227/aa10227.html|bibcode = 2001A&A...368...16M |doi-access=free}}</ref> Its [[galaxy disk|spiral disk]] is of type III and there is a dust structure which is more prominent to the east.<ref>{{cite journal|last1=Gutiérrez|first1=Leonel|last2=Erwin|first2=Peter|last3=Aladro|first3=Rebeca|last4=Beckman|first4=John E.|title=The Outer Disks of Early-type Galaxies. II. Surface-brightness Profiles of Unbarred Galaxies and Trends with Hubble Type|journal=The Astronomical Journal|date=1 November 2011|volume=142|issue=5|pages=145|doi=10.1088/0004-6256/142/5/145|arxiv = 1108.3662 |bibcode = 2011AJ....142..145G |s2cid=118386795}}</ref> The galaxy features two ring structures, with diameter 1.62 and 2.42 arcminutes.<ref>{{cite journal|last1=Comerón|first1=S.|last2=Salo|first2=H.|last3=Laurikainen|first3=E.|last4=Knapen|first4=J. H.|last5=Buta|first5=R. J.|last6=Herrera-Endoqui|first6=M.|last7=Laine|first7=J.|last8=Holwerda|first8=B. W.|last9=Sheth|first9=K.|last10=Regan|first10=M. W.|last11=Hinz|first11=J. L.|last12=Muñoz-Mateos|first12=J. C.|last13=Gil de Paz|first13=A.|last14=Menéndez-Delmestre|first14=K.|last15=Seibert|first15=M.|last16=Mizusawa|first16=T.|last17=Kim|first17=T.|last18=Erroz-Ferrer|first18=S.|last19=Gadotti|first19=D. A.|last20=Athanassoula|first20=E.|author20-link=Lia Athanassoula|last21=Bosma|first21=A.|last22=Ho|first22=L. C.|title=ARRAKIS: atlas of resonance rings as known in the S4G|journal=Astronomy & Astrophysics|date=19 February 2014|volume=562|pages=A121|doi=10.1051/0004-6361/201321633|arxiv = 1312.0866 |bibcode = 2014A&A...562A.121C |s2cid=119295831}}</ref> The [[spiral arm]]s are tightly wound and form an inner pseudoring and they continue for one revolution outside the ring. The outer arms are very patchy and filamentary.<ref>{{cite journal|last1=Eskridge|first1=Paul B.|last2=Frogel|first2=Jay A.|last3=Pogge|first3=Richard W.|last4=Quillen|first4=Alice C.|last5=Berlind|first5=Andreas A.|last6=Davies|first6=Roger L.|last7=DePoy|first7=D. L.|last8=Gilbert|first8=Karoline M.|last9=Houdashelt|first9=Mark L.|last10=Kuchinski|first10=Leslie E.|last11=Ramirez|first11=Solange V.|last12=Sellgren|first12=K.|last13=Stutz|first13=Amelia|last14=Terndrup|first14=Donald M.|last15=Tiede|first15=Glenn P.|title=Near-Infrared and Optical Morphology of Spiral Galaxies|journal=The Astrophysical Journal Supplement Series|date=November 2002|volume=143|issue=1|pages=73–111|doi=10.1086/342340|arxiv = astro-ph/0206320 |bibcode = 2002ApJS..143...73E |s2cid=15491635}}</ref>


One [[supernova]] has been observed in NGC 3675: SN 1984R (type unknown, mag. 13) was discovered by [[Kaoru Ikeya]] on 2 December 1984.<ref>{{cite journal | bibcode = 1984IAUC.4021....1K| title = Possible Supernova in NGC 3675| last1 = Kosai| first1 = H.| last2 = Ikeya| first2 = K.| last3 = Shibasaki| first3 = H.| journal = International Astronomical Union Circular| date = 1984| issue = 4021| page = 1}}</ref><ref>{{cite web | website=Transient Name Server | title=SN{{nbsp}}1984R | url=https://www.wis-tns.org/object/1984R | publisher = [[International_Astronomical_Union|IAU]] | access-date=5 December 2024}}</ref>
One [[supernova]] has been observed in NGC 3675, SN 1984R. NGC 3675 belongs to the [[Ursa Major Cluster]], part of the [[Virgo Supercluster]].<ref>{{cite web|title=The Ursa Major Groups|url=http://www.atlasoftheuniverse.com/galgrps/uma.html|website=www.atlasoftheuniverse.com}}</ref>


== Gallery ==
== Gallery ==
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Ngc3675-hst-R658GB814.jpg|NGC 3675 ([[Hubble Space Telescope|HST]])
Ngc3675-hst-R658GB814.jpg|NGC 3675 ([[Hubble Space Telescope|HST]])
</gallery>
</gallery>

== See also ==
* [[List of NGC objects (3001–4000)]]


== References ==
== References ==
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{{commonscat}}
{{commonscat}}
{{wikiSky}}
{{wikiSky}}



{{Ngc40}}
{{Ngc40}}
{{Catalogs|NGC=3675}}
{{Ursa Major}}


[[Category:Unbarred spiral galaxies]]
[[Category:Unbarred spiral galaxies]]
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[[Category:NGC objects|3675]]
[[Category:NGC objects|3675]]
[[Category:UGC objects|06439]]
[[Category:UGC objects|06439]]
[[Category:Principal Galaxies Catalogue objects|35164]]
[[Category:Principal Galaxies Catalogue objects|035164]]
[[Category:MCG objects|+07-24-004]]
[[Category:IRAS catalogue objects|11234+4351]]
[[Category:Astronomical objects discovered in 1788|17880114]]
[[Category:Discoveries by William Herschel]]

Latest revision as of 03:02, 6 December 2024

NGC 3675
NGC 3675 in Schulman telescope
Observation data (J2000 epoch)
ConstellationUrsa Major
Right ascension11h 26m 08.5689s[1]
Declination+43° 35′ 09.696″[1]
Redshift0.002568[1]
Heliocentric radial velocity770 ± 1 km/s[1]
Distance53 ± 10 Mly (16.2 ± 3.0 Mpc)[1]
Apparent magnitude (V)10.0
Characteristics
TypeSA(s)b [1]
Size~105,700 ly (32.41 kpc) (estimated)[1]
Apparent size (V)5.9′ × 3.1′[1]
Other designations
IRAS 11234+4351, UGC 6439, MCG +07-24-004, PGC 35164, CGCG 214-005[1]

NGC 3675 is a spiral galaxy located in the constellation Ursa Major. It is located at a distance of about 50 million light years from Earth, which, given its apparent dimensions, means that NGC 3675 is about 100,000 light years across. It was discovered by German-British astronomer William Herschel on 14 January 1788.[2] NGC 3675 belongs to the Ursa Major Cluster, part of the Virgo Supercluster.[3]

It hosts a low-ionization nuclear emission-line region (LINER).[4] In the nucleus there is a supermassive black hole with an estimated mass of 10-39 million M☉, based on the intrinsic velocity dispersion as measured by the Hubble Space Telescope.[5] Although the galaxy was reported to have a strong bar visible in infrared images, there has been no indication of a bar in further observations.[6] Its spiral disk is of type III and there is a dust structure which is more prominent to the east.[7] The galaxy features two ring structures, with diameter 1.62 and 2.42 arcminutes.[8] The spiral arms are tightly wound and form an inner pseudoring and they continue for one revolution outside the ring. The outer arms are very patchy and filamentary.[9]

One supernova has been observed in NGC 3675: SN 1984R (type unknown, mag. 13) was discovered by Kaoru Ikeya on 2 December 1984.[10][11]

[edit]
  • NGC 3675 (SDSS DR14)
    NGC 3675 (SDSS DR14)
  • NGC 3675 (HST)
    NGC 3675 (HST)

See also

[edit]

References

[edit]
  1. ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for object NGC 3675. Retrieved 2016-01-18.
  2. ^ Seligman, Courtney. "New General Catalogue Objects: NGC 3675". Celestial Atlas. Retrieved 5 December 2024.
  3. ^ "The Ursa Major Groups". www.atlasoftheuniverse.com.
  4. ^ McKernan, B.; Ford, K. E. S.; Reynolds, C. S. (20 July 2010). "Black hole mass, host galaxy classification and AGN activity". Monthly Notices of the Royal Astronomical Society. 407 (4): 2399–2410. arXiv:1005.4907. Bibcode:2010MNRAS.407.2399M. doi:10.1111/j.1365-2966.2010.17068.x. S2CID 118679872.
  5. ^ Beifiori, A.; Sarzi, M.; Corsini, E. M.; Bontà, E. Dalla; Pizzella, A.; Coccato, L.; Bertola, F. (10 February 2009). "Upper Limits on the Masses of 105 Supermassive Black Holes from Hubble Space Telescope/Space Telescope Imaging Spectrograph Archival Data". The Astrophysical Journal. 692 (1): 856–868. arXiv:0809.5103. Bibcode:2009ApJ...692..856B. doi:10.1088/0004-637X/692/1/856. S2CID 54903233.
  6. ^ Möllenhoff, C.; Heidt, J. (15 March 2001). "Surface photometry of spiral galaxies in NIR:Structural parameters of disks and bulges". Astronomy & Astrophysics. 368 (1): 16–37. Bibcode:2001A&A...368...16M. doi:10.1051/0004-6361:20000335.
  7. ^ Gutiérrez, Leonel; Erwin, Peter; Aladro, Rebeca; Beckman, John E. (1 November 2011). "The Outer Disks of Early-type Galaxies. II. Surface-brightness Profiles of Unbarred Galaxies and Trends with Hubble Type". The Astronomical Journal. 142 (5): 145. arXiv:1108.3662. Bibcode:2011AJ....142..145G. doi:10.1088/0004-6256/142/5/145. S2CID 118386795.
  8. ^ Comerón, S.; Salo, H.; Laurikainen, E.; Knapen, J. H.; Buta, R. J.; Herrera-Endoqui, M.; Laine, J.; Holwerda, B. W.; Sheth, K.; Regan, M. W.; Hinz, J. L.; Muñoz-Mateos, J. C.; Gil de Paz, A.; Menéndez-Delmestre, K.; Seibert, M.; Mizusawa, T.; Kim, T.; Erroz-Ferrer, S.; Gadotti, D. A.; Athanassoula, E.; Bosma, A.; Ho, L. C. (19 February 2014). "ARRAKIS: atlas of resonance rings as known in the S4G". Astronomy & Astrophysics. 562: A121. arXiv:1312.0866. Bibcode:2014A&A...562A.121C. doi:10.1051/0004-6361/201321633. S2CID 119295831.
  9. ^ Eskridge, Paul B.; Frogel, Jay A.; Pogge, Richard W.; Quillen, Alice C.; Berlind, Andreas A.; Davies, Roger L.; DePoy, D. L.; Gilbert, Karoline M.; Houdashelt, Mark L.; Kuchinski, Leslie E.; Ramirez, Solange V.; Sellgren, K.; Stutz, Amelia; Terndrup, Donald M.; Tiede, Glenn P. (November 2002). "Near-Infrared and Optical Morphology of Spiral Galaxies". The Astrophysical Journal Supplement Series. 143 (1): 73–111. arXiv:astro-ph/0206320. Bibcode:2002ApJS..143...73E. doi:10.1086/342340. S2CID 15491635.
  10. ^ Kosai, H.; Ikeya, K.; Shibasaki, H. (1984). "Possible Supernova in NGC 3675". International Astronomical Union Circular (4021): 1. Bibcode:1984IAUC.4021....1K.
  11. ^ "SN 1984R". Transient Name Server. IAU. Retrieved 5 December 2024.
[edit]
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