2004/02/29 by G. E. Romero, I. A Grenier, M. M. Kaufman Bernado +2
Physics and Astronomy · #astro-ph
published as ESA Spec.Publ. 552 (2004) 703-707 · Paper presented at the fifth INTEGRAL workshop. 4 pages, 4 figures. Includes small changes requested by the referee
arxiv created 2004/04/21 · arxiv updated 2009/12/01
Some phenomenological properties of the unidentified EGRET detections suggest that there are two distinct groups of galactic gamma-ray sources that might be associated with compact objects endowed with relativistic jets. We discuss different models for gamma-ray production in both microquasars with low- and high-mass stellar companions. We conclude that the parent population of low-latitude and halo variable sources might be formed by yet undetected microquasars and microblazars.