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Chemical Evolution of Elliptical Galaxies and the ICM

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Preprint , Other literature type 01 Jan 2003Embargo end date: 01 Jan 2002Publisher:Springer NetherlandsJournal:Astrophysics and Space Science, volume 284, pages 799-802 (issn: 0004-640X, eissn: 1572-946X,

Authors: Francesca Matteucci; Antonio Pipino;

doi: 10.1007/978-94-017-3315-1_101 , 10.1023/a:1024037727520 , 10.48550/arxiv.astro-ph/0210542

arXiv: http://arxiv.org/abs/astro-ph/0210542

Chemical Evolution of Elliptical Galaxies and the ICM

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Abstract

We present a new model for the chemical evolution of elliptical galaxies taking into account SN feedback, detailed nucleosynthesis and galactic winds. We discuss the effect of galactic winds on the chemical enrichment of the ICM and compute the energy per particle injected by the galaxies into the ICM.

4 pages, 2 figures, to appear in the ''Proceedings of The evolution of galaxies III. From simple approaches to self-consistent models'', Kiel (Germany), 2002

Related Organizations

University of Trieste
Italy

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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