An introduction to the pair-reflection model of X-ray spectra in AGN's

Details An introduction to the pair-reflection model of X-ray spectra in AGN's An introduction to the pair-reflection model of X-ray spectra in AGN's

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992xrea.conf..103s&link_type=abstract

In MPI für Extraterrestrische Physik, X Ray Emission from Active Galactic Nuclei and the Cosmic X Ray Background p 103-116 (SEE

Mathematics

6

Active Galactic Nuclei, Gamma Ray Spectra, Pair Production, Stellar Models, X Ray Spectra, Emission Spectra, Extreme Ultraviolet Radiation, Mathematical Models, Nonthermal Radiation, Robustness (Mathematics), Variability

Scientific paper

The pair reflection model of Zdziarski, Ghisellini, George, Svensson, Fabian, and Done (1990), in which most features of the extreme ultraviolet gamma ray spectra of Active Galactic Nuclei (AGN) are accounted for is considered. Details of the conception of the model are given and the model itself is explained. In the pair reflection model a pair cloud located above a cold slab generates a self consistently computed nonthermal spectrum that irradiates and is reflected by the slab. Some of these features are discussed using simplest possible arguments. The robustness of the pair reflection model as well as possible variability patterns are also discussed.

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