Production of the diffuse X-ray background spectrum by active galactic nuclei

Details Production of the diffuse X-ray background spectrum by active galactic nuclei Production of the diffuse X-ray background spectrum by active galactic nuclei

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...332..157s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 332, Sept. 1, 1988, p. 157-162.

Astronomy and Astrophysics

Astrophysics

47

Active Galactic Nuclei, Background Radiation, Bremsstrahlung, X Ray Sources, X Ray Spectra, Luminosity, Red Shift

Scientific paper

The authors propose a class of models in which the intensity and spectrum of the X-ray background radiation between 0.2 and 160 keV can be produced by active galactic nuclei. The key assumption of these models is that the spectra of active galactic nuclei are not described by a single power law. No evolution of the X-ray spectra of active galactic nuclei is required.

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