Blue supergiant
A blue supergiant (BSG ) is a hot, luminous star , also called an OB supergiant . They are usually thought to be those with luminosity class I and spectral class B9 or earlier, although sometimes A-class supergiants are also called blue supergiants.
They are bigger than the Sun but smaller than a red supergiant , with surface temperatures of 10,000–50,000 K and luminosities from about 10,000 to a million times that of the Sun. They might form when two stars merge together.
References
↑ Massey, P.; Puls, J.; Pauldrach, A. W. A.; Bresolin, F.; Kudritzki, R. P.; Simon, T. (2005). "The Physical Properties and Effective Temperature Scale of O-Type Stars as a Function of Metallicity. II. Analysis of 20 More Magellanic Cloud Stars and Results from the Complete Sample" . The Astrophysical Journal . 627 (1): 477– 519. arXiv :astro-ph/0503464 . Bibcode :2005ApJ...627..477M . doi :10.1086/430417 . S2CID 18172086 .
↑ Yüce, Kutluay (2005-01-01). "Spectral Analysis of 4 Lacertae and ν Cephei" . Baltic Astronomy . 14 : 51– 82. Bibcode :2005BaltA..14...51Y . ISSN 1021-6766 .
↑ Burgos, A. de; Simon-Díaz, S.; Lennon, D. J.; Dorda, R.; Negueruela, I.; Urbaneja, M. A.; Patrick, L. R.; Herrero, A. (2020-11-01). "High-resolution spectroscopic study of massive blue and red supergiants in Perseus OB1 - I. Definition of the sample, membership, and kinematics" . Astronomy & Astrophysics . 643 : A116. arXiv :2008.13299 . Bibcode :2020A& A...643A.116D . doi :10.1051/0004-6361/202039019 . ISSN 0004-6361 .
↑ Wagle, Gururaj A.; Ray, Alak; Raghu, Adarsh (May 2020). "Type IIP Supernova Progenitors. III. Blue to Red Supergiant Ratio in Low-metallicity Models with Convective Overshoot" . The Astrophysical Journal . 894 (2): 118. arXiv :2004.14419 . Bibcode :2020ApJ...894..118W . doi :10.3847/1538-4357/ab8bd5 . ISSN 0004-637X .
↑ Menon, Athira; Ercolino, Andrea; Urbaneja, Miguel A.; Lennon, Daniel J.; Herrero, Artemio; Hirai, Ryosuke; Langer, Norbert; Schootemeijer, Abel; Chatzopoulos, Emmanouil; Frank, Juhan; Shiber, Sagiv (March 2024). "Evidence for Evolved Stellar Binary Mergers in Observed B-type Blue Supergiants" . The Astrophysical Journal Letters . 963 (2): L42. Bibcode :2024ApJ...963L..42M . doi :10.3847/2041-8213/ad2074 . ISSN 2041-8205 .
↑ Galaxy v23n06 (1965 08) .
↑ Koberlein, Brian (2024-03-26). "Merging Stars Can Lead to Blue Supergiants" . Universe Today . Retrieved 2024-03-28 .