X-ray Statistics of WR Colliding-Wind Binaries

被引:0
|
作者
Kogure, Tomokazu [1 ]
机构
[1] Kyoto Univ, Kyoto 6148322, Japan
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STARS;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Statistical correltation between X-ray luminosity and orbital priod of WR + O binaries which are suspected to have strong colliding-wind activities is considered. Results show that, short-period binaries have similar X-ray luminosity with single WR, stars, while binary stars with long-period and high eccentricity can be strong X-ray emitter at some phase of orbital motion.
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页码:212 / 214
页数:3
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