EAS Publications Series
Volume 24, 2007CRAL-2006. Chemodynamics: From First Stars to Local Galaxies
|Page(s)||139 - 144|
|Published online||21 April 2007|
E. Emsellem, H. Wozniak, G. Massacrier, J.-F. Gonzalez, J. Devriendt and N. Champavert (eds)
EAS Publications Series, 24 (2007) 139-144
Chemical enrichment of galaxy clusters from hydrodynamical simulations
SISSA – International School for Advanced Studies, Trieste, Italy
2 Dipartimento di Astronomia, Università di Trieste, Italy
Corresponding author: firstname.lastname@example.org
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.
© EAS, EDP Sciences, 2007
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.