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astro-ph2000
A code for optically thick and hot photoionized media
A. -M. Dumont, A. Abrassart, S. Collin
We describe a code designed for hot media {(T } a few 10 K), optically thick to Compton scattering. It computes the structure of a plane-parallel slab of gas in thermal an…
astro-ph2000
X-ray emitting-absorbing media in Seyfert 1 galaxies
M. Mouchet, A. Abrassart, D. Porquet +2
Seyfert galaxies have been shown to exhibit a large variety of features in their X-ray spectra from which the environment of the central engine can be deduced. We focus on the two…
astro-ph2000
Accretion and Emission Processes in AGN: the UV-X Connection
S. Collin, A. Abrassart, B. Czerny +2
The main characteristics of the average spectrum of radio quiet AGN in the UV and X-ray range are reviewed, and the emission mechanisms are discussed in the framework of accretion…