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MWC 656: A Be+BH or a Be+sdO?
Published online by Cambridge University Press: 29 August 2024
Abstract
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MWC 656 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.
- Type
- Poster Paper
- Information
- Proceedings of the International Astronomical Union , Volume 18 , Symposium S361: Massive Stars Near and Far , May 2022 , pp. 332 - 333
- Copyright
- © The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union
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