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Cluster Formation with Chemical and Energy Feedback

Published online by Cambridge University Press:  26 May 2016

L. Portinari ,
J. Sommer-Larsen  and
A. D. Romeo
L. Portinari
Affiliation:
Theoretical Astrophysics Center, Juliane Maries Vej 30, Copenhagen, Denmark
J. Sommer-Larsen
Affiliation:
Theoretical Astrophysics Center, Juliane Maries Vej 30, Copenhagen, Denmark
A. D. Romeo
Affiliation:
Theoretical Astrophysics Center, Juliane Maries Vej 30, Copenhagen, Denmark

Abstract

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We present fully cosmological, hydrodynamical simulations of clusters of galaxies, including star formation, supernova feedback, chemical enrichment and metal-dependent cooling. We investigate the relation between feedback, metal enrichment of the intra-cluster medium (ICM) and the distribution of baryons in the various phases (cold gas+stars and hot ICM) at varying Initial Mass Function and wind efficiency.

Type
Part 3. Ejection and Outflow
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 328 - 330
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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