Relativistic Neutrons in Active Galactic Nuclei - Part Two - Gamma-Rays of High and Very High Energies

Details Relativistic Neutrons in Active Galactic Nuclei - Part Two - Gamma-Rays of High and Very High Energies Relativistic Neutrons in Active Galactic Nuclei - Part Two - Gamma-Rays of High and Very High Energies

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...257..476a&link_type=abstract

Astronomy and Astrophysics, Vol. 257, NO. 2/APR(II), P. 476, 1992

Astronomy and Astrophysics

Astrophysics

10

Scientific paper

In the frames of the AGN model proposed in Paper I the problem of the electromagnetic cascade initiated in a spatially non-homogeneous field of background photons due to propagation of relativistic neutrons (RNs) from the proton acceleration region r <= r_0_ ~ 10 and their decay at large radii, r_0_= 1 TeV) gamma-rays from the bright extragalactic sources with relatively low luminosities L_mx_ < 10^45^ erg s^-1^.

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