Exploration of spin-down rate of neutron stars in high-mass X-ray binaries
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/457/4/3889/18510744/stw111.pdf
Reference62 articles.
1. Maximum mass-loss rates of line-driven winds of massive stars
2. Gamma-rays from the vicinity of accreting neutron stars inside compact high-mass X-ray binaries
3. Observations of Accreting Pulsars
4. On the Mechanism of Accretion by Stars
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1. Studies of Cepheus X-4 during the 2018 Outburst Observed with AstroSat;The Astrophysical Journal;2021-10-01
2. Spin evolution of neutron stars in wind-fed high-mass X-ray binaries;Publications of the Astronomical Society of Japan;2020-09-19
3. On the possibility of disk-fed formation in supergiant high-mass X-ray binaries;Research in Astronomy and Astrophysics;2019-01
4. CAN THE SUBSONIC ACCRETION MODEL EXPLAIN THE SPIN PERIOD DISTRIBUTION OF WIND-FED X-RAY PULSARS?;The Astrophysical Journal;2016-06-22
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