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The Chemical Evolution of the Intra-Cluster Medium

Published online by Cambridge University Press:  26 May 2016

Wilfried Domainko ,
Wolfgang Kapferer ,
Sabine Schindler ,
Eelco van Kampen ,
Stefan Kimeswenger  and
Maximilian Ruffert
Wilfried Domainko
Affiliation:
Institut für Astrophysik, Leopold-Franzens-Universität Innsbruck Technikerstraße 25, A-6020 Innsbruck, Austria
Wolfgang Kapferer
Affiliation:
Institut für Astrophysik, Leopold-Franzens-Universität Innsbruck Technikerstraße 25, A-6020 Innsbruck, Austria
Sabine Schindler
Affiliation:
Institut für Astrophysik, Leopold-Franzens-Universität Innsbruck Technikerstraße 25, A-6020 Innsbruck, Austria
Eelco van Kampen
Affiliation:
Institut für Astrophysik, Leopold-Franzens-Universität Innsbruck Technikerstraße 25, A-6020 Innsbruck, Austria
Stefan Kimeswenger
Affiliation:
Institut für Astrophysik, Leopold-Franzens-Universität Innsbruck Technikerstraße 25, A-6020 Innsbruck, Austria
Maximilian Ruffert
Affiliation:
Department for Mathematics and Statistics, University of Edinburgh JCMB, Mayfield Road, Edinburgh, EH9 3JZ, UK

Abstract

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We present numerical simulations of the dynamical and chemical evolution of galaxy clusters. from X-ray spectra it is evident that the Intra-Cluster Medium (ICM) is abundant in metals. As heavy elements are only produced in stars the processed material must have been ejected by cluster galaxies into the ICM. Several different mechanisms for interaction between the cluster galaxies and the ICM are possible but their efficiency of metal enrichment of the cluster and their time evolution are still not known. Suggested processes which remove enriched material from the galaxies are ram-pressure stripping, galactic winds, superwinds driven by starburst activity and jets from active galaxies. First results of high resolution hydrodynamic simulations on cluster scales are presented to investigate the effect of these different pollution mechanisms.

Type
Part 3. Ejection and Outflow
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 464 - 465
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Collela, P., Woodward, P.R., 1984, J. Comput. Phys., 54, 174.Google Scholar
Gunn, J.E., Gott, J.R. III, 1972, ApJ, 176, 1.Google Scholar
van Kampen, E., Jimenez, R., Peacock, J. A., 1999, MNRAS, 310, 43.Google Scholar
Ruffert, M., 1992, A&A, 265, 82.Google Scholar