Neutrinos from Blazars and the Differences between FRI and FRII Radio Galaxies

Details Neutrinos from Blazars and the Differences between FRI and FRII Radio Galaxies Neutrinos from Blazars and the Differences between FRI and FRII Radio Galaxies

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...199.6807d&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #68.07; Bulletin of the American Astronomical Society, Vol. 33, p.1413

Astronomy and Astrophysics

Astronomy

Scientific paper

Nonthermal proton acceleration in galaxy jets produce neutrinos through photomeson production. Sources with intense surrounding fields should be strong neutrino sources. Neutrons and high-energy photons formed through photomeson processes will transport inner jet energy far from the black hole engine to power distant jets, hot spots and lobes, as observed at X-ray energies with Chandra. This effect may account for differences between the FRI and FRII classes of radio galaxies that display distinct morphologies.

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