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dc.contributor.authorCea del Pozo, Elsa de-
dc.contributor.authorTorres, Diego F.-
dc.contributor.authorRodríguez, Ana Yaiza-
dc.date.accessioned2009-02-20T10:16:06Z-
dc.date.available2009-02-20T10:16:06Z-
dc.date.issued2009-01-18-
dc.identifier.citationarXiv:0901.2688v1 [astro-ph.GA]en_US
dc.identifier.urihttp://hdl.handle.net/10261/10852-
dc.description14 pages, 5 figures.en_US
dc.description.abstractIn this paper, a consistent model of the multifrequency emission of the starburst galaxy M82, from radio to gamma-rays, and neutrinos, is presented and discussed. Predictions for Fermi, MAGIC II/VERITAS and CTA telescopes are made. The model is used to self-consistenty compute the emission of neutrinos resulting from this starburst galaxy, what can be used in considerations of the diffuse contributions of such objects.en_US
dc.description.sponsorshipWe acknowledge support by grants AYA 2006-00530, CSIC-PIE 200750I029, and AYA2008- 01181-E/ESP. The work of E. de Cea del Pozo has been made under the auspice of a FPI Fellowship, grant BES-2007-15131.en_US
dc.format.extent452156 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoengen_US
dc.relation.isversionofPreprint-
dc.rightsopenAccessen_US
dc.subjectStarburst galaxy M82en_US
dc.subjectMultifrequency emissionen_US
dc.subjectNeutrinosen_US
dc.subjectGamma raysen_US
dc.subjectRadioen_US
dc.subjectGalaxy astrophysicsen_US
dc.titleMulti-messenger model for the starburst galaxy M82en_US
dc.typepreprinten_US
dc.description.peerreviewedPeer revieweden_US
dc.relation.publisherversionhttp://arxiv.org/abs/0901.2688en_US
dc.type.coarhttp://purl.org/coar/resource_type/c_816bes_ES
item.languageiso639-1en-
item.fulltextWith Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_816b-
item.cerifentitytypePublications-
item.grantfulltextopen-
item.openairetypepreprint-
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