A chemical evolution model for galaxy clusters

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dc.creatorPortinari, L.
dc.creatorMoretti, A.
dc.creatorChiosi, C.
dc.date2001-08-05
dc.date.accessioned2026-07-07T01:59:33Z
dc.date.available2026-07-07T01:59:33Z
dc.descriptionWe develop a toy-model for the chemical evolution of the intracluster medium, polluted by the galactic winds from elliptical galaxies. The model follows the "galaxy formation history" of cluster galaxies, constrained by the observed luminosity function.
dc.description6 pages, 10 figures, to appear in the Proceedings of the Workshop "Chemical Enrichment of Intracluster and Intergalactic Medium", Vulcano, Italy, 14-18 May 2001, ASP Conference Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0108077
dc.identifierhttp://arxiv.org/abs/astro-ph/0108077
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3159
dc.subjectAstrophysics
dc.titleA chemical evolution model for galaxy clusters
dc.typetext

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