Stellar wind accretion and accretion disk formation: Applications to neutron star high-mass X-ray binaries

Author:

Karino Shigeyuki1,Nakamura Kenji2,Taani Ali3

Affiliation:

1. Faculty of Science and Engineering, Kyushu Sangyo University, 2-3-1 Matsukadai, Higashi-ku, Fukuoka, Fukuoka 813-8503, Japan

2. Department of Mechanical Engineering, Kyushu Sangyo University, 2-3-1 Matsukadai, Higashi-ku, Fukuoka, Fukuoka 813-8503, Japan

3. Physics Department, Faculty of Science, Al-Balqa Applied University, 19117 Salt, Jordan

Funder

JSPS

Institute of High Energy Physics

Chinese Academy of Sciences

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 21 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Rapid population synthesis of black hole high-mass X-ray binaries: implications for binary stellar evolution;Monthly Notices of the Royal Astronomical Society;2023-06-15

2. Torque reversals and wind variations of X-ray pulsar Vela X-1;Monthly Notices of the Royal Astronomical Society: Letters;2022-10-07

3. The Chemical Nature of Orion Protostars: Are ORANGES Different from PEACHES? ORANGES II.;The Astrophysical Journal;2022-04-01

4. Possible TeV Gamma-Ray Binary Origin of HESS J1828–099;The Astrophysical Journal Letters;2022-03-01

5. Determination of wind-fed model parameters of neutron stars in high-mass X-ray binaries;Publications of the Astronomical Society of Australia;2022

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