Astronomy and Astrophysics – Astronomy
Scientific paper
May 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990natur.345..319g&link_type=abstract
Nature (ISSN 0028-0836), vol. 345, May 24, 1990, p. 319-322.
Astronomy and Astrophysics
Astronomy
30
Active Galactic Nuclei, Neutrons, Radio Sources (Astronomy), Relativistic Particles, Astronomical Spectroscopy, Electron Density (Concentration), Emission Spectra, Field Strength, Synchrotron Radiation
Scientific paper
The intensity spectrum of the core of radio-loud AGN varies smoothly from 10 exp 8.5 to 10 to the 16th Hz, and is flat between 10 to the 9th and 10 to the 10th Hz, implying that a single emission mechanism is responsible. It is proposed here that energy is transported from the central source by relativistic neutrons which travel freely over a large volume and decay into relativistic protons. The protons produce secondary electrons which generate the observed radiation. The photon spectra thus produced are largely model-independent and flat.
Giovanoni Peter M.
Kazanas Demosthenes
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