A nonthermal model for the XUV, soft X-ray emission of AGN and QSOs

Details A nonthermal model for the XUV, soft X-ray emission of AGN and QSOs A nonthermal model for the XUV, soft X-ray emission of AGN and QSOs

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...320l...1j&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 320, Sept. 1, 1987, p. L1-L4.

Astronomy and Astrophysics

Astrophysics

14

Active Galactic Nuclei, Extreme Ultraviolet Radiation, Galactic Radiation, Quasars, Synchrotron Radiation, X Rays, Emission Spectra, Heao 2, Photoionization

Scientific paper

XUV and soft X-ray radiation of active galactic nuclei may be explained
by synchrotron emission of secondary electrons resulting from pp
collisions in the vicinity of a supermassive compact object. The
spectrum would be the natural extension of the ultraviolet emission
responsible for photoionization of the emission-line gas.

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