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Chemical enrichment of galaxy clusters from hydrodynamical simulations

Published online by Cambridge University Press:  21 April 2007

E. Emsellem ,
H. Wozniak ,
G. Massacrier ,
J.-F. Gonzalez ,
J. Devriendt ,
N. Champavert ,
L. Tornatore  and
S. Borgani
L. Tornatore*
Affiliation:
SISSA – International School for Advanced Studies, Trieste, Italy
S. Borgani
Affiliation:
Dipartimento di Astronomia, Università di Trieste, Italy
*
[email protected]
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Abstract

We have developed in GADGET-2 a feature–rich and highly flexible code for modeling the stellar evolution and the chemical enrichment. Simulating clusters, we find a very good agreement in reproducing both the radial abundance profiles and the enrichment history of the Intra–Cluster medium.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 24: CRAL-2006. Chemodynamics: From First Stars to Local Galaxies , 2007 , pp. 139 - 144
Copyright
© EAS, EDP Sciences, 2007

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