A comparison between the radio and the X-ray spectra of broad-line radio galaxies

Details A comparison between the radio and the X-ray spectra of broad-line radio galaxies A comparison between the radio and the X-ray spectra of broad-line radio galaxies

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1085..522a&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: Proceedings of the 4th International Meeting on High Energy Gamma-Ray Astronomy. AIP Conferenc

Astronomy and Astrophysics

Astronomy

1

Radio Galaxies, X-Ray, Galactic Nuclei, Circumnuclear Matter, And Bulges

Scientific paper

We present the spectral characteristics of a sample of Intermediate-Luminosity Broad-Line Radio Galaxies in X-rays, optical and radio. Here, we focus on the radio spectra acquired with the 100 m radio telescope in Effelsberg between 2.6 GHz and 32 GHz. These measurements reveal different spectral shapes urging for radio imaging that would disclose the source morphology. Comparing them with the X-ray spectra acquired with XMM-Newton, we find that sources with steep radio spectrum are heavily obscured whereas flat spectrum ones appear unabsorbed in accordance with unified scheme.

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