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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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Bibliografische Detailangaben
Hauptverfasser: Yu-Dong Nie, Yong Shao, Jian-Guo He, Ze-Lin Wei, Xiao-Jie Xu, Xiang-Dong Li
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2025-01-01
Schriftenreihe:The Astrophysical Journal
Schlagworte:
Online-Zugang:https://doi.org/10.3847/1538-4357/ad9a65
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