Broad band properties of radio-loud emission line AGNs

Details Broad band properties of radio-loud emission line AGNs Broad band properties of radio-loud emission line AGNs

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..510..382g&link_type=abstract

THE FIFTH COMPTON SYMPOSIUM. AIP Conference Proceedings, Volume 510, pp. 382-386 (2000).

Physics

Active And Peculiar Galaxies And Related Systems, Radiation Mechanisms, Polarization

Scientific paper

Recent BeppoSAX observations of bright radio galaxies have shown that they have a considerable variety of spectral properties and important differences with respect to Seyfert galaxies. Reprocessing features (Fe line and reflection hump) are not always present and generally weak. We suggest two possible scenarios: either radio-loud objects have disk X-ray emission diluted by the jet, or their X-ray reprocessing material subtends a smaller solid angle because of different accretion disk geometry and physical characteristics. .

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