The cosmic ray luminosity of the nearby active galactic nuclei

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dc.creatorDedenko, L. G.
dc.creatorPodgrudkov, D. A.
dc.creatorRoganova, T. M.
dc.creatorFedorova, G. F.
dc.date2008-04-29
dc.date.accessioned2026-07-07T09:35:50Z
dc.date.available2026-07-07T09:35:50Z
dc.descriptionThe pointing directions of extensive air showers observed at the Pierre Auger Observatory were fitted within 3.1 degree with positions of the nearby active galactic nuclei from the Veron-Cetty and P. Veron catalog. The cosmic ray luminosity of the active galactic nuclei which happened to be a source of the particular cosmic ray event constitutes a fraction ~0.0001 of the optical one if only cosmic ray particles with energies above 60 EeV are produced. If produced cosmic ray particles have a spectrum dE/E^3 up to ~100 GeV then the cosmic ray luminosity would be much higher than the optical one of the active galactic nuclei.
dc.description9 pages, 5 figures, 1 table
dc.identifierhttps://arxiv.org/abs/0804.4582
dc.identifierhttp://arxiv.org/abs/0804.4582
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/159964
dc.subjectAstrophysics
dc.titleThe cosmic ray luminosity of the nearby active galactic nuclei
dc.typetext

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