DM clumps as discrete sources of gamma-radiation

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dc.creatorBelotsky, K. M.
dc.creatorGalper, A. M.
dc.date2005-07-06
dc.date.accessioned2026-07-07T02:18:11Z
dc.date.available2026-07-07T02:18:11Z
dc.descriptionMassive objects (clumps) of Cold Dark Matter (CDM) in Galaxy can appear due to its annihilation as discrete sources of gamma-radiation. Some number of unidentified regular gamma-sources, observed by EGRET, can be accounted for by massive CDM clumps. Future gamma-ray expreriment GLAST in combination with data of EGRET will enable to probe a wide range of models of clumped annihilating CDM.
dc.description4 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0507118
dc.identifierhttp://arxiv.org/abs/astro-ph/0507118
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9394
dc.subjectAstrophysics
dc.titleDM clumps as discrete sources of gamma-radiation
dc.typetext

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