High energy processes in microquasars

被引：0
|
作者：
Paredes, JM [1 ]
机构：
[1] Univ Barcelona, Dept Astron & Meteorol, E-08028 Barcelona, Spain
来源：
HIGH ENERGY GAMMA-RAY ASTRONOMY | 2005年 / 745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：
Microquasars are X-ray binary stars with the capability to generate relativistic jets. It is expected that microquasars are gamma-ray sources, because of the analogy with quasars and because the theoretical models predict emission at such energy range. In addition, from observational arguments, there are two microquasars that appear as the possible counterparts for two unidentified high-energy gamma-ray sources.
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页码：93 / 104
页数：12
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