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

来源：

SPACE SCIENCE REVIEWS | 1994年 / 69卷 / 3-4期

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

页码：255 / 329

页数：75

共 277 条

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