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

Paola Grandi·Giorgio G. C. Palumbo
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Abstract

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.

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Paola Grandi, Giorgio G. C. Palumbo. 2006-11-10. Broad Line Radio Galaxies: Jet Contribution to the nuclear X-Ray Continuum. https://doi.org/10.1063/1.2757339

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