1995/09/07 by K. Mannheim, M. Schulte, J. Rachen
Physics and Astronomy · #astro-ph
published as Astron.Astrophys. 303 (1995) L41 · 4 pages, uuencoded and compressed Postscript file, also available at http://www.uni-sw.gwdg.de/preprints/preprints.html
arxiv created 1995/09/07 · arxiv updated 2009/12/01
We predict that the UV bump spectrum of quasars extends into the soft X-ray range with a steep power law. For radio-louds, the spectral index is alphas ~ 1.7 (Snu = So nu-alpha), and for radio-quiets it should be somewhat steeper alphas >~ 1.7. The prediction is based on a simple scenario in which all quasars, radio-quiets and radio-louds, are assumed to have jets close to their accretion disks. Soft X-rays are produced via unsaturated Comptonization of UV photons from the disk in the (marginally) optically thick jet base. Nonthermal hard X-rays are produced further downstream. The scenario requires that (i) the jet kinetic luminosity is always of the same order as the UV luminosity and (ii) that the nonthermal radiative efficiency is ~ 10%. In radio-quiets, the jets should have speeds of ~ 0.3c and a low Mach number leading to rapid decollimation and turbulent mass entrainment within the central parsec.