Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-11-10
AIPConf.Proc.921:335-336,2007
Astronomy and Astrophysics
Astrophysics
12 pages including 2 figures (4 files), ApJ accepted
Scientific paper
10.1063/1.2757339
It 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.
Grandi Paola
Palumbo Giorgio G. C.
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