Is there a connection between non-synchronous rotation and X-ray emission in massive binary systems

被引：0
|
作者：
Haro, S [1 ]
Juárez, JA
Koenigsberger, G
机构：
[1] Univ Nacl Autonoma Mexico, Inst Astron, Mexico City 04510, DF, Mexico
[2] Univ Nacl Autonoma Mexico, Ctr Ciencias Fis, Cuernavaca 62251, Morelos, Mexico
来源：
STELLAR ROTATION | 2004年 / 215期
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A correlation between orbital period and log(L-X/L-bol) is found for a sample of B-type binary systems. We suggest that wind-wind collisions are the likely mechanism for generating the X-ray emission: and that the mass-loss rates may be enhanced in non-synchronously rotating systems due to the oscillations that are excited by the tidal forces.
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页码：163 / 165
页数：3
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