A Compton reflection model for the cosmic X-ray and gamma-ray backgrounds

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Background Radiation, Compton Effect, Cosmic X Rays, Endeavour (Orbiter), Gamma Rays, X Ray Sources, Astronomical Models, Gamma Ray Spectra, Reflected Waves, Spectrum Analysis

Scientific paper

The gamma-ray spectrum of an AGN in the Compton reflection model is calculated and the contribution of such sources to the cosmic gamma-ray background is considered. The spectrum is composed of three parts: an X-ray power law, a broad hump from roughly 10 to 120 keV due to reprocessing of the power-law X-ray spectrum by cold gas, and gamma rays which are due to the inverse-Compton scattering of X-rays. The contribution of such sources to the cosmic gamma-ray background is computed and it is found that they provide an excellent fit to the entire background spectrum from 3 keV to 10 MeV. Constraints on the physical conditions in these sources are derived based on these results and the possibility of observing such sources with GRO is considered.

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