AGNs and microquasars as high-energy gamma-ray sources

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dc.contributor.authorParedes i Poy, Josep Maria
dc.date.accessioned2013-08-27T07:55:18Z
dc.date.available2013-08-27T07:55:18Z
dc.date.issued2005
dc.date.updated2013-08-27T07:55:18Z
dc.description.abstractThe 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.
dc.format.extent8 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec546712
dc.identifier.issn0004-640X
dc.identifier.urihttps://hdl.handle.net/2445/45384
dc.language.isoeng
dc.publisherSpringer Science + Business Media
dc.relation.isformatofVersió postprint del document publicat a: http;//dx.doi.org/10.1007/s10509-005-1177-8
dc.relation.ispartofAstrophysics and Space Science, 2005, vol. 300, num. 1-3, p. 267-274
dc.relation.urihttp://dx.doi.org/10.1007/s10509-005-1177-8
dc.rights(c) Springer Science + Business Media, 2005
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationEstels binaris de raigs X
dc.subject.classificationRaigs gamma
dc.subject.classificationAstronomia de raigs gamma
dc.subject.classificationQuàsars
dc.subject.otherX-ray binaries
dc.subject.otherGamma rays
dc.subject.otherGamma ray astronomy
dc.subject.otherQuasars
dc.titleAGNs and microquasars as high-energy gamma-ray sources
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/acceptedVersion

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