The X-ray Emission and the Magnetic Fields of Late-Type Stars

被引：0
|
作者：
J.R. Shi
G. Zhao
Y. Zhao
机构：
[1] Chinese Academy of Sciences,National Astronomical Observatories
[2] Chinese Academy of Science Peking University joint Beijing Astrophysical Center,undefined
来源：
Astrophysics and Space Science | 2002年 / 282卷
关键词：
Coronal Heating; Active Star; Program Star; Coronal Temperature; Hardness Ratio;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
We present the results of X-ray luminosities of some active late-type stars, based on data primarily from the ROSAT position sensitive proportional counter (PSPC). According to the observations, we divide the stars into four groups: single, wide binary, binary and RS CVn. We investigated the correlation between the X-ray emission and the hardness ratio, coronal temperature, magnetic field strength, magnetic flux density. Our results suggest that the magnetic field plays a very important role in stellar X-ray emission.
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页码：477 / 488
页数：11
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