http://arxiv.org/abs/2208.12315
MWC656 has been reported as classical Be star with a black hole companion. Revisited spectral variability properties render this unlikely, with a hot subdwarf more probable.
T. Rivinius, R. Klement, S. Chojnowski, et. al.
Mon, 29 Aug 22
24/49
Comments: To be published in IAUS361 proceedings
You must be logged in to post a comment.