Spectral-luminosity evolution of active galactic nuclei (AGN)

Details Spectral-luminosity evolution of active galactic nuclei (AGN) Spectral-luminosity evolution of active galactic nuclei (AGN)

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..254..370l&link_type=abstract

In: Testing the AGN paradigm; Proceedings of the 2nd Annual Topical Astrophysics Conference, Univ. of Maryland, College Park, Oc

Astronomy and Astrophysics

Astrophysics

2

Accretion Disks, Active Galactic Nuclei, Cosmic X Rays, Gamma Ray Spectra, Luminosity, X Ray Spectra, Background Radiation, Red Shift, Scattering Cross Sections, Thomson Scattering

Scientific paper

The origin of the cosmic X-ray and gamma-ray backgrounds is explained
via the mechanism of AGN spectral-luminosity evolution. The spectral
evolution of precursor active galaxies into AGN, and Newton-Raphson
input and output parameters are discussed.

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