The intrinsic high metallicity of cSNRs

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dc.creatorRodriguez-Gonzalez, A.
dc.creatorTenorio-Tagle, G.
dc.creatorSilich, S.
dc.date2003-03-13
dc.date.accessioned2026-07-07T02:07:53Z
dc.date.available2026-07-07T02:07:53Z
dc.descriptionHere we present semi-analytical solutions of the hydrodynamics of compact supernova remnants (cSNRs) and their chemical evolution. Two models of $15 M_{\odot}$ and $25 M_{\odot}$ supernova explosions evolving in a high density medium ($n_0 \sim 10^7 cm^{-3}$) are throughly discussed.
dc.description4 pages, 3 figures, Accepted for publication in Revista Mexicana de Astronomia & Astrofisica
dc.identifierhttps://arxiv.org/abs/astro-ph/0303276
dc.identifierhttp://arxiv.org/abs/astro-ph/0303276
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5849
dc.subjectAstrophysics
dc.titleThe intrinsic high metallicity of cSNRs
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