The effect of the Galactic gas distribution on the expected cosmic rays spectrum

Simple item page
dc.creatorMollá, M.
dc.creatorAguilar, M.
dc.creatorAlcaraz, J.
dc.creatorBerdugo, J.
dc.creatorCasaus, J.
dc.creatorDiaz, C.
dc.creatorLanciotti, E.
dc.creatorMañá, C.
dc.creatorMarin, J.
dc.creatorMartinez, G.
dc.creatorPalomares, C.
dc.creatorSánchez, E.
dc.creatorSevilla, I.
dc.creatorTorrentó, A. S.
dc.date2004-11-25
dc.date.accessioned2026-07-07T02:16:02Z
dc.date.available2026-07-07T02:16:02Z
dc.descriptionWe will analyze the importance of varying the diffuse gas radial distribution on the resulting expected cosmic rays spectrum. We use the recent HI density data published by Nakanishi et al. (2004), and include them in the cosmic rays propagation code GALPROP (Strong & Moskalenko 1998). We will obtain those models that reproduce the characteristics shown by the cosmic rays data, and we will then extract information about the Galaxy structure.
dc.descriptionto appear in ESO Astrophysics Symposia: Exploring the Cosmic Frontier
dc.identifierhttps://arxiv.org/abs/astro-ph/0411692
dc.identifierhttp://arxiv.org/abs/astro-ph/0411692
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8635
dc.subjectAstrophysics
dc.titleThe effect of the Galactic gas distribution on the expected cosmic rays spectrum
dc.typetext

Files

Collections

arXiv