High Energy Neutrinos from Blazars

Simple item page
dc.creatorProtheroe, R. J.
dc.date1996-07-31
dc.date.accessioned2026-07-07T02:21:41Z
dc.date.available2026-07-07T02:21:41Z
dc.descriptionI describe a model of energetic gamma ray and neutrino emission in blazars which is consistent with most of the gamma-ray observations, and use this model to estimate the diffuse intensity of high energy neutrinos from blazars.
dc.description4 pages, 2 figures, to appear in Accretion Phenomena and Related Outflows, IAU Colloq. 163, ed. D. Wickramashinghe et al., 1996
dc.identifierhttps://arxiv.org/abs/astro-ph/9607165
dc.identifierhttp://arxiv.org/abs/astro-ph/9607165
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10596
dc.subjectAstrophysics
dc.titleHigh Energy Neutrinos from Blazars
dc.typetext

Files

Collections

arXiv