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

Bibliographic Details
Title: Modeling High Mass X-Ray Binaries to Double Neutron Stars through Common Envelope Evolution
Authors: Yu-Dong Nie, Yong Shao, Jian-Guo He, Ze-Lin Wei, Xiao-Jie Xu, Xiang-Dong Li
Source: The Astrophysical Journal, Vol 979, Iss 2, p 112 (2025)
Publisher Information: IOP Publishing, 2025.
Publication Year: 2025
Collection: LCC:Astrophysics
Subject Terms: Binary stars, Neutron stars, Stellar evolution, X-ray binary stars, Supernovae, Astrophysics, QB460-466
More Details: 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 evolution and consider various CE ejection efficiencies varying in the range of 0.1–3.0. We focus on the evolutionary consequences of the binaries that survived CE evolution. We demonstrate that it is possible for the binaries to enter a CE decoupling phase (CEDP) when the donor stars are partially stripped, leaving a hydrogen envelope of ≲1.0–4.0 M _⊙ after CE evolution. This phase is expected to last ∼10 ^4 –10 ^5 yr, during which mass transfer occurs stably via Roche lobe overflow with super-Eddington rates. Identification of some X-ray binaries in a CEDP is important for the understanding of the physics of CE evolution itself, the origin of ultraluminous X-ray sources, and the recycling process of accreting pulsars. Also, we discuss the formation of double neutron stars and the occurrence of ultrastripped supernovae according to the results from our simulations. On the whole, the properties of post-CE binaries are sensitive to the options of CE ejection efficiencies.
Document Type: article
File Description: electronic resource
Language: English
ISSN: 1538-4357
Relation: https://doaj.org/toc/1538-4357
DOI: 10.3847/1538-4357/ad9a65
Access URL: https://doaj.org/article/c261fa32b2f64769ab5a11442e7f0a4e
Accession Number: edsdoj.261fa32b2f64769ab5a11442e7f0a4e
Database: Directory of Open Access Journals
More Details
ISSN:15384357
DOI:10.3847/1538-4357/ad9a65
Published in:The Astrophysical Journal
Language:English