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

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

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.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Broad Line Radio Galaxies: Jet Contribution to the nuclear X-Ray Continuum does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Broad Line Radio Galaxies: Jet Contribution to the nuclear X-Ray Continuum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Broad Line Radio Galaxies: Jet Contribution to the nuclear X-Ray Continuum will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-565547

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.