Modeling High Mass X-Ray Binaries to Double Neutron Stars through Common Envelope Evolution

We present detailed evolutionary simulations of wide binary systems with high-mass (8–20 M _⊙ ) donor stars and a 1.4 M _⊙ neutron star. Mass transfer in such binaries is dynamically unstable, and common envelope (CE) evolution is followed. We use a recently developed prescription to deal with CE ev...

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Bibliographic Details
Main Authors: Yu-Dong Nie, Yong Shao, Jian-Guo He, Ze-Lin Wei, Xiao-Jie Xu, Xiang-Dong Li
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/ad9a65
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