The radio to hard X-ray spectral energy distribution of BeppoSAX emission line AGN

Details The radio to hard X-ray spectral energy distribution of BeppoSAX emission line AGN The radio to hard X-ray spectral energy distribution of BeppoSAX emission line AGN

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..599..738m&link_type=abstract

X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background. Edited by Nicholas E. White, Giuseppe Malaguti, and G

Astronomy and Astrophysics

Astronomy

Galactic Nuclei, Circumnuclear Matter, And Bulges, Radio Sources, X-Ray Sources, X-Ray Bursts

Scientific paper

We have studied the correlation between the hard X-ray (10 keV) luminosity, the radio (5GHz) luminosity and the [OIII]5007 Å luminosity in an heterogeneous sample of emission line AGN observed by BeppoSAX. We find strong correlations between all these luminosities. We also find that the [OIII]5007 luminosity is correlated with the ratio between the 10 keV and the 5 GHz luminosity at the 98% confidence level. This suggests that the [OIII] emission is probably not related only to the UV ionizing radiation from the AGN, and therefore that the [OIII] emission is not a perfect indicator of the isotropic UV radiation field. .

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