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AGNS and MICROQUASARS As High-Energy γ-Ray Sources
Authors:Josep M Paredes
Institution:(1) Departament d'Astronomia i Meteorologia, Universitat de Barcelona, Av. Diagonal 647, 08028 Barcelona, 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.
Keywords:X-rays: binaries  stars: individual: LS 5039  LS I +61 303  gamma-rays: observations
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