Bosch i Ramon, ValentíParedes i Poy, Josep Maria2013-08-272013-08-2720051009-9271https://hdl.handle.net/2445/45391The possible associations between the microquasars LS 5039 and LS I +61 303 and the EGRET sources 3EG J1824-1514 and 3EG J0241+6103 suggest that microquasars could also be sources of high-energy gamma-rays. In this work, we present a detailed numerical inverse Compton (IC) model, based on a microquasar scenario, that reproduces the high-energy gamma-ray spectra and variability observed by EGRET for the mentioned sources. Our model considers a population of relativistic electrons entrained in a cylindrical inhomogeneous jet that interact through IC scattering with both the radiation and the magnetic fields.6 p.application/pdfeng(c) Chinese Academy of Sciences, 2005Estels binaris de raigs XEstelsRaigs gammaAstronomia de raigs XAstrofísicaX-ray binariesStarsGamma raysX-ray astronomyAstrophysicsinfo:eu-repo/semantics/article5176542013-08-27info:eu-repo/semantics/openAccess