Hostname: page-component-6bf8c574d5-r8w4l Total loading time: 0 Render date: 2025-03-08T02:27:26.456Z Has data issue: false hasContentIssue false
  • English
  • Français

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]
Get access

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

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)