AGNS and MICROQUASARS As High-Energy γ-Ray Sources
DOI: 10.1007/s10509-005-1177-8
Bibcode: 2005Ap&SS.300..267P
Paredes, Josep M.
Spain
Abstract
The extragalactic analogs of the microquasars, the quasars, are strong γ-ray emitters at GeV energies. It is expected that microquasars are also γ-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 γ-ray sources.
2005
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Astrophysics and Space Science
INTEGRAL
3