Sources of Cosmic Rays and Galactic Diffuse Gamma Radiation

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dc.creatorCasanova, Sabrina
dc.creatorBiermann, Peter L.
dc.creatorEngel, Ralph
dc.creatorMeli, Athina
dc.creatorUlrich, Ralf
dc.date2004-03-29
dc.date.accessioned2026-07-07T02:12:45Z
dc.date.available2026-07-07T02:12:45Z
dc.descriptionThe diffuse galactic gamma-ray spectrum measured by the EGRET experiment \citep{Hunter:1997} are interpreted within a scenario in which cosmic rays (CRs) are injected by three different kind of sources, (i) supernovae (SN) which explode into the interstellar medium (ISM), (ii) Red Supergiants (RSG), and (iii) Wolf-Rayet stars (WR), where the two latter explode into their pre-SN winds (Biermann et al. 2001; Sina et al. 2001).
dc.descriptionINTEGRAL workshop 2004 in Munich, 4 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0403661
dc.identifierhttp://arxiv.org/abs/astro-ph/0403661
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7566
dc.subjectAstrophysics
dc.titleSources of Cosmic Rays and Galactic Diffuse Gamma Radiation
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