X-RAY-EMISSION FROM BE STAR X-RAY BINARIES

被引:29
作者
APPARAO, KMV
机构
[1] Tata Institute of Fundamental Research, Colaba, 400 005, Bombay, Homi Bhabha Road
关键词
D O I
10.1007/BF02101698
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Observations of X-ray emission from Be star/X-ray binaries are reviewed. Some optical characteristics of these binaries are also presented. Theoretical aspects pertaining to the X-ray emissions are given.
引用
收藏
页码:255 / 329
页数:75
相关论文
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