High-energy gamma-ray emission from microquasars: LS 5039 and LS I+61303

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dc.contributor.authorBosch i Ramon, Valentí
dc.contributor.authorParedes i Poy, Josep Maria
dc.date.accessioned2013-08-27T11:23:18Z
dc.date.available2013-08-27T11:23:18Z
dc.date.issued2005
dc.date.updated2013-08-27T11:23:18Z
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.extent6 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec517654
dc.identifier.issn1009-9271
dc.identifier.urihttps://hdl.handle.net/2445/45391
dc.language.isoeng
dc.publisherChinese Academy of Sciences
dc.relation.isformatofVersió postprint del document publicat a: http://dx.doi.org/10.1088/1009-9271/5/S1/133
dc.relation.ispartofChinese Journal of Astronomy and Astrophysics, 2005, vol. 5, p. 133-138
dc.relation.urihttp://dx.doi.org/10.1088/1009-9271/5/S1/133
dc.rights(c) Chinese Academy of Sciences, 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.classificationEstels
dc.subject.classificationRaigs gamma
dc.subject.classificationAstronomia de raigs X
dc.subject.classificationAstrofísica
dc.subject.otherX-ray binaries
dc.subject.otherStars
dc.subject.otherGamma rays
dc.subject.otherX-ray astronomy
dc.subject.otherAstrophysics
dc.titleHigh-energy gamma-ray emission from microquasars: LS 5039 and LS I+61303
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/acceptedVersion

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