UHECR Anisotropy from Luminous Infrared Galaxies - Predictions for the Pierre Auger Observatory

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dc.creatorMaria, Giller
dc.creatorWojciech, Michalak
dc.creatorAndrzej, Smialkowski
dc.date2003-08-29
dc.date.accessioned2026-07-07T02:09:20Z
dc.date.available2026-07-07T02:09:20Z
dc.descriptionWe consider the hypothesis that luminous infrared galaxies (LIRGs) are sources of the UHECRs. By associating the AGASA triplet with the Arp 299 galaxy we obtain reasonable values for Galactic and extragalactic magnetic fields. We predict what the southern sky, to be seen by the Auger experiment, should look like, so that the LIRG hypothesis could be verified soon.
dc.descriptionTalk given at 28th International Cosmic Ray Conference, Tsukuba, Japan, 31 jul- 7 aug 2003
dc.identifierhttps://arxiv.org/abs/astro-ph/0308532
dc.identifierhttp://arxiv.org/abs/astro-ph/0308532
dc.identifierProceedings of the 28th ICRC, Tsukuba, Japan, (2003), p.727
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6397
dc.subjectAstrophysics
dc.titleUHECR Anisotropy from Luminous Infrared Galaxies - Predictions for the Pierre Auger Observatory
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