ROTATION OF CLOSE BINARY-SYSTEM COMPONENTS

被引：3
|
作者：
MEREZHIN, VP
机构：
[1] State Institute of Applied Optics, Kazan
来源：
ASTROPHYSICS AND SPACE SCIENCE | 1994年 / 218卷 / 02期
关键词：
D O I：
10.1007/BF00627761
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The rotation of close binary system components is investigated. The principal physical characteristics as well as the equatorial rotational velocities and th e axial and orbital inclinations for 46 close binary systems were determined. It is found that the rotation axes of the individual stars in a pair cross the orbital plane under different angles. As a rule, the rotation and orbital periods of a vast majority of the systems investigated here do not coincide.
引用
收藏
页码：223 / 248
页数：26
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