天鵝座BI

天鵝座BI （BI Cyg”、IRC +40408、BD+36 4025）是在天鵝座的一顆紅超巨星。它是一顆不規則變星，最大亮度為星等8.4，最暗星等9.9。 它被認為是天鹅座OB1星協的成員，距離太陽系大約2,600秒差距（8,500光年）。它位於另一個也是變星的紅超巨星天鵝座BC以南不到一度的地方。 天鵝座BI是一顆慢不規則變星，被歸類為Lc型，一顆不規則的超巨星。 它的亮度極值在星等8.4和9.9等之間變化。其光變曲線的頻率分析顯示沒有顯著的週期。 天鵝座BI是已知最大的恆星之一，基於3,575K的有效溫度和226,000 L☉，其半徑大約是1,240 R☉。最近的研究得出的亮度較低，低於 130,000 L☉，建議其初始量質為20 M☉，因此半徑值也較低。 天鵝座RW 天鵝座KY 天鵝座NML Vallenari, A.; et al. Gaia Data Release 3. Summary of the content and survey properties. Astronomy & Astrophysics. 2022. arXiv:2208.00211 . doi:10.1051/0004-6361/202243940 .  已忽略未知参数|collaboration= (帮助) Gaia DR3 record for this source at VizieR. 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.  Bailer-Jones, C. A. L.; Rybizki, J.; Fouesneau, M.; Demleitner, M.; Andrae, R. Estimating Distances from Parallaxes. V. Geometric and Photogeometric Distances to 1.47 Billion Stars in Gaia Early Data Release 3. The Astronomical Journal. 2021, 161 (3): 147. Bibcode:2021AJ....161..147B. S2CID 228063812. arXiv:2012.05220 . doi:10.3847/1538-3881/abd806.  Table 4 in Levesque, Emily M.; Massey, Philip; Olsen, K. A. G.; Plez, Bertrand; Josselin, Eric; Maeder, Andre; Meynet, Georges. The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not As Cool As We Thought. The Astrophysical Journal. August 2005, 628 (2): 973–985. Bibcode:2005ApJ...628..973L. S2CID 15109583. arXiv:astro-ph/0504337 . doi:10.1086/430901.  Anders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A.; Matijevič, G.; Monari, G.; Cantat-Gaudin, T.; Weiler, M.; Khan, S.; Miglio, A.; Carrillo, I.; Romero-Gómez, M.; Minchev, I.; De Jong, R. S.; Antoja, T.; Ramos, P.; Steinmetz, M.; Enke, H. Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18. Astronomy and Astrophysics. 2019, 628: A94. Bibcode:2019A&A...628A..94A. S2CID 131780028. arXiv:1904.11302 . doi:10.1051/0004-6361/201935765.  Comerón, F.; Djupvik, A. A.; Schneider, N.; Pasquali, A. The historical record of massive star formation in Cygnus. Astronomy & Astrophysics. October 2020, 2009: A62. Bibcode:2020A&A...644A..62C. S2CID 221970180. arXiv:2009.12779 . doi:10.1051/0004-6361/202039188.  Messineo, M.; Brown, A. G. A. A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2. The Astronomical Journal. 2019, 158 (1): 20. Bibcode:2019AJ....158...20M. S2CID 148571616. arXiv:1905.03744 . doi:10.3847/1538-3881/ab1cbd.  Norris, Ryan P. Seeing Stars Like Never Before: A Long-term Interferometric Imaging Survey of Red Supergiants (PDF) (学位论文). Georgia State University. 2019 [2023-08-14]. （原始内容存档 (PDF)于2022-01-24）.  OMC Archive. OMC Archive. The Astronomical Data Centre at CAB. [19 December 2021]. （原始内容存档于2022-11-30）.  Kiss, L. L; Szabó, Gy. M; Bedding, T. R. Variability in red supergiant stars: Pulsations, long secondary periods and convection noise. Monthly Notices of the Royal Astronomical Society. 2006, 372 (4): 1721–1734. Bibcode:2006MNRAS.372.1721K. S2CID 5203133. arXiv:astro-ph/0608438 . doi:10.1111/j.1365-2966.2006.10973.x.  Nicolas Mauron; Eric Josselin. The mass-loss rates of red supergiants and the de Jager prescription. Astronomy and Astrophysics. 2010, 526: A156. Bibcode:2011A&A...526A.156M. S2CID 119276502. arXiv:1010.5369 . doi:10.1051/0004-6361/201013993.  Josselin, E.; Plez, B. Atmospheric dynamics and the mass loss process in red supergiant stars. Astronomy and Astrophysics. 2007, 469 (2): 671–680. Bibcode:2007A&A...469..671J. S2CID 17789027. arXiv:0705.0266 . doi:10.1051/0004-6361:20066353.  INTEGRAL-OMC Catalogue of optically variable sources （页面存档备份，存于互联网档案馆）