A Channel to Form Fast-spinning Black Hole–Neutron Star Binary Mergers as Multimessenger Sources. II. Accretion-induced Spin-up

A Channel to Form Fast-spinning Black Hole–Neutron Star Binary Mergers as Multimessenger Sources. II. Accretion-induced Spin-up

In this work, we investigate an alternative channel for the formation of fast-spinning black hole–neutron star (BHNS) binaries, in which super-Eddington accretion is expected to occur in accreting BHs during the stable mass transfer phase within BH-stripped helium (BH–He-rich) star binary systems. W...

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Bibliographic Details
Main Authors: Zhen-Han-Tao Wang, Rui-Chong Hu, Ying Qin, Jin-Ping Zhu, Bing Zhang, Shuang-Xi Yi, Qin-Wen Tang, Xin-Wen Shu, Fen Lyu, En-Wei Liang
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Gravitational waves
Close binary stars
Black holes
Neutron stars
Online Access:https://doi.org/10.3847/1538-4357/ad2fc1

Internet

https://doi.org/10.3847/1538-4357/ad2fc1

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