AGNs and microquasars as high-energy γ-ray sources

被引：5

作者：

Paredes, JM ^{[1
]}

机构：

[1] Univ Barcelona, Dept Astron & Meteorol, E-08028 Barcelona, Spain

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2005年 / 300卷 / 1-3期

关键词：

X-rays : binaries; stars : individual : LS 5039; LS I+61 303; gamma-rays : observations;

D O I：

10.1007/s10509-005-1177-8

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The extragalactic analogs of the microquasars, the quasars, are strong gamma-ray emitters at GeV energies. It is expected that microquasars are also gamma-ray sources, because of the analogy with quasars and because theoretical models predict the high-energy emission. There are two microquasars that appear as the possible counterparts for two unidentified high-energy gamma-ray sources.

引用

页码：267 / 274

页数：8

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