Unidentified Gamma-Ray Sources and Microquasars

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dc.creatorRomero, G. E.
dc.creatorGrenier, I. A
dc.creatorBernado, M. M. Kaufman
dc.creatorMirabel, I. F.
dc.creatorTorres, D. F.
dc.date2004-02-12
dc.date2004-04-21
dc.date.accessioned2026-07-07T02:12:15Z
dc.date.available2026-07-07T02:12:15Z
dc.descriptionSome 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.
dc.descriptionPaper presented at the fifth INTEGRAL workshop. 4 pages, 4 figures. Includes small changes requested by the referee
dc.identifierhttps://arxiv.org/abs/astro-ph/0402285
dc.identifierhttp://arxiv.org/abs/astro-ph/0402285
dc.identifierESA Spec.Publ. 552 (2004) 703-707
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7386
dc.subjectAstrophysics
dc.titleUnidentified Gamma-Ray Sources and Microquasars
dc.typetext

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