Hard X-ray emission from colliding stellar winds

被引：0
|
作者：
Bychkov, KV
Seifina, EV
机构：
来源：
ASTRONOMICHESKII ZHURNAL | 1996年 / 73卷 / 05期
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A theoretical analysis of the emission from colliding stellar winds in binary systems is conducted. The fraction of emission from the region surrounding the ram point increases with energy of the emitted quanta; therefore, it is most convenient to determine the flow parameters from observations in the hard X-ray range (E > 10 keV).
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页码：735 / 739
页数：5
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