Broad Band Spectral Analysis Of Nine Radio Bright Type 1 AGN Detected By INTEGRAL
Abstract
Broad Line Radio Galaxies (BLRG) are, in AGN Unified Schemes, the radio loud counterparts of Seyfert 1 galaxies. They show similar optical/UV characteristics, but have different behaviours in the X-ray domain. They show, in fact, harder power law slopes and weaker reprocessing features than their radio quiet counterparts. In this poster we present the broad band (1-150 keV) spectral analysis of nine radio bright AGN detected by INTEGRAL together with XMM- Newton, Swift/XRT and Chandra data. In a number of sources we were able to constrain the cut-off energy and/or the reflection component. We also compare our findings to radio quiet type 1 objects detected by INTEGRAL and discuss them in the light of current unified models. The sources analysed here all show a remarkable similarity with radio quiet type 1 objects, with only slightly weaker reprocessing features. Our findings also suggest that some other mechanism could be present that inhibits strong reflection components and does not favour the dilution of the AGN component.
- Publication:
-
37th COSPAR Scientific Assembly
- Pub Date:
- 2008
- Bibcode:
- 2008cosp...37.2084M