Broad Line Radio Galaxies: Jet Contribution to the nuclear X-Ray Continuum

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dc.creatorGrandi, Paola
dc.creatorPalumbo, Giorgio G. C.
dc.date2006-11-10
dc.date.accessioned2026-07-07T11:00:09Z
dc.date.available2026-07-07T11:00:09Z
dc.descriptionIt is shown that, for Broad Line Radio Galaxies the strength of the non-thermal beamed radiation, when present, is always smaller than the accretion flow by a factor < 0.7 in the 2-10 keV band. The result has been obtained using the procedure adopted for disentangling the Flat Spectrum Radio Quasar 3C 273 (Grandi & Palumbo 2004). Although this implies a significantly smaller non-thermal flux in Radio Galaxies when compared to Blazars, the jet component, if present, could be important at very high energies and thus easily detectable with GLAST.
dc.description12 pages including 2 figures (4 files), ApJ accepted
dc.identifierhttps://arxiv.org/abs/astro-ph/0611342
dc.identifierhttp://arxiv.org/abs/astro-ph/0611342
dc.identifierAIPConf.Proc.921:335-336,2007
dc.identifierdoi:10.1063/1.2757339
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/187624
dc.subjectAstrophysics
dc.titleBroad Line Radio Galaxies: Jet Contribution to the nuclear X-Ray Continuum
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