SPIN EVOLUTION IN WIND-FED X-RAY BINARIES

被引：8

作者：

KING, AR

机构：

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1991年 / 250卷 / 02期

关键词：

D O I：

10.1093/mnras/250.1.3P

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Global angular momentum balance suggests that the neutron stars in Be/X-ray binaries are not spinning in equilibrium. This requires an X-ray lifetime less-than-or-similar-to 10(5) yr, and suggests that there are many 'dead' Be/X-ray binaries in the Galaxy. Some of these may be turned up as millisecond radio pulsars with Be star campanions.

引用

页码：P3 / P4

页数：2

共 10 条

[1]

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[2]

CORBET R, 1985, SPACE SCI REV, V40, P409

[3]

CORBET RHD, 1984, ASTRON ASTROPHYS, V141, P91

[4] THE 3 TYPES OF HIGH-MASS X-RAY PULSATOR [J].