HD 180314: Difference between revisions
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'''HD 180314''' is a [[star]] in the constellation [[Lyra]]. Its apparent magnitude is 6.61. The star is orbited by one substellar companion,<ref name=SIMBAD>{{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?IdentHD+180314&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id |title = HD 180314|work = SIMBAD Astronomical Database|publisher=Centre de Données astronomiques de Strasbourg |accessdate = 22 February 2014}}</ref> an object with a minimum mass 22 times that of [[Jupiter]] and hence likely to be a [[brown dwarf]].<ref name="sato 2010">{{cite journal|author=Sato, Bun'ei; Omiya, Masashi; Liu, Yujuan; Harakawa, Hiroki; Izumiura, Hideyuki; Kambe, Eiji; Toyota, Eri; Murata, Daisuke; Lee, Byeong-Cheol; Masuda, Seiji; Takeda, Yoichi; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro; Ida, Shigeru; Zhao, Gang; Han, Inwoo;|date=2010|title=Substellar Companions to Evolved Intermediate-Mass Stars: HD 145457 and HD 180314|journal=Publications of the Astronomical Society of Japan|volume=62|issue=4|pages=1063–69|bibcode=2010PASJ...62.1063S|doi=10.1093/pasj/62.4.1063}}</ref> |
'''HD 180314''' is a [[star]] in the constellation [[Lyra]]. Its apparent magnitude is 6.61. The star is orbited by one substellar companion,<ref name=SIMBAD>{{cite web |url =http://simbad.u-strasbg.fr/simbad/sim-id?IdentHD+180314&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id |title = HD 180314|work = SIMBAD Astronomical Database|publisher=Centre de Données astronomiques de Strasbourg |accessdate = 22 February 2014}}</ref> an object with a minimum mass 22 times that of [[Jupiter]] and hence likely to be a [[brown dwarf]].<ref name="sato 2010">{{cite journal|author=Sato, Bun'ei; Omiya, Masashi; Liu, Yujuan; Harakawa, Hiroki; Izumiura, Hideyuki; Kambe, Eiji; Toyota, Eri; Murata, Daisuke; Lee, Byeong-Cheol; Masuda, Seiji; Takeda, Yoichi; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro; Ida, Shigeru; Zhao, Gang; Han, Inwoo;|date=2010|title=Substellar Companions to Evolved Intermediate-Mass Stars: HD 145457 and HD 180314|journal=Publications of the Astronomical Society of Japan|volume=62|issue=4|pages=1063–69|bibcode=2010PASJ...62.1063S|doi=10.1093/pasj/62.4.1063|arxiv = 1005.2860 }}</ref> |
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==References== |
==References== |
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Revision as of 17:14, 9 May 2015
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Lyra |
| Right ascension | 19h 14m 50.20890s [1] |
| Declination | +31° 51′ 37.2569″ [1] |
| Spectral type | K0III |
HD 180314 is a star in the constellation Lyra. Its apparent magnitude is 6.61. The star is orbited by one substellar companion,[1] an object with a minimum mass 22 times that of Jupiter and hence likely to be a brown dwarf.[2]
References
- ^ a b c "HD 180314". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 22 February 2014.
- ^ Sato, Bun'ei; Omiya, Masashi; Liu, Yujuan; Harakawa, Hiroki; Izumiura, Hideyuki; Kambe, Eiji; Toyota, Eri; Murata, Daisuke; Lee, Byeong-Cheol; Masuda, Seiji; Takeda, Yoichi; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro; Ida, Shigeru; Zhao, Gang; Han, Inwoo; (2010). "Substellar Companions to Evolved Intermediate-Mass Stars: HD 145457 and HD 180314". Publications of the Astronomical Society of Japan. 62 (4): 1063–69. arXiv:1005.2860. Bibcode:2010PASJ...62.1063S. doi:10.1093/pasj/62.4.1063.
{{cite journal}}: CS1 maint: extra punctuation (link) CS1 maint: multiple names: authors list (link)
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