Spin evolution of long-period X-ray pulsars

被引：0
|
作者：
N. R. Ikhsanov
Yu. S. Likh
N. G. Beskrovnaya
机构：
[1] Russian Academy of Sciences,Central (Pulkovo) Astronomical Observatory
[2] St. Petersburg State University,undefined
来源：
Astronomy Reports | 2014年 / 58卷
关键词：
Neutron Star; Astronomy Report; Stellar Wind; Equilibrium Period; Spin Period;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
The spin evolution of X-ray pulsars in high-mass X-ray binaries is discussed under various assumptions about the geometry and physical parameters of the accretion flow. The torque applied to the neutron star by the accretion flow and the equilibrium periods of the pulsars are estimated. It is shown that the observed spin evolution of the pulsars can be explained in a scenario in which the neutron star accretes material from a magnetized stellar wind.
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页码：376 / 385
页数：9
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