A nova-like red variable in M31
作者： Jeremy Mould , Judith Cohen , James R. Graham , Don Hamilton , Keith Matthews
DOI: 10.1086/185702
关键词: Red supergiant 、 Luminous red nova 、 Astrophysics 、 Apparent magnitude 、 Bulge 、 Astronomy 、 Supergiant 、 Giant star 、 Physics 、 Light curve 、 Variable star 、 Space and Planetary Science 、 Astronomy and Astrophysics
摘要: A late-type supergiant which appeared in the bulge of M31 last observing season faded 3 bolometric magnitudes 100 days and is now no longer detectable. It suggested that object was a nova an unusual type. 9 refs.
harvard.edu
sci-hub.st 参考文章(0)