X-ray emission from isolated Be stars

被引：0
|
作者：
Cohen, DH [1 ]
机构：
[1] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA
来源：
BE PHENOMENON IN EARLY-TYPE STARS, PROCEEDINGS | 2000年 / 175卷
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：
I discuss the X-ray observations of Be stars, and how their properties compare to non-emission B stars. I focus on several specific stars that show high flux levels and variability but also report on several interesting survey results. The Be X-ray properties are discussed in the context of wind-shock X-ray emission from normal OB stars as well as in the context of general mechanisms that have been proposed to explain the Be phenomenon. Finally, I conclude with a discussion of the spectral diagnostics that will be available from the new generation of X-ray telescopes.
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页码：156 / 169
页数：4
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