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Enrichment of the intracluster medium from infalling galaxies

Published online by Cambridge University Press:  06 October 2004

Eelco van Kampen ,
Wilfried Domainko ,
Wolfgang Kapferer ,
Sabine Schindler ,
Stefan Kimeswenger ,
Otonyo Mangete  and
Max Ruffert
Eelco van Kampen
Affiliation:
Institute for Astrophysics, University of Innsbruck Technikerstraße 25, A-6020 Innsbruck, AustriaEelco.v.Kampen@uibk.ac.at http://astro.uibk.ac.at/astroneu/hydroskiteam/index.htm
Wilfried Domainko
Affiliation:
Institute for Astrophysics, University of Innsbruck Technikerstraße 25, A-6020 Innsbruck, AustriaEelco.v.Kampen@uibk.ac.at http://astro.uibk.ac.at/astroneu/hydroskiteam/index.htm
Wolfgang Kapferer
Affiliation:
Institute for Astrophysics, University of Innsbruck Technikerstraße 25, A-6020 Innsbruck, AustriaEelco.v.Kampen@uibk.ac.at http://astro.uibk.ac.at/astroneu/hydroskiteam/index.htm
Sabine Schindler
Affiliation:
Institute for Astrophysics, University of Innsbruck Technikerstraße 25, A-6020 Innsbruck, AustriaEelco.v.Kampen@uibk.ac.at http://astro.uibk.ac.at/astroneu/hydroskiteam/index.htm
Stefan Kimeswenger
Affiliation:
Institute for Astrophysics, University of Innsbruck Technikerstraße 25, A-6020 Innsbruck, AustriaEelco.v.Kampen@uibk.ac.at http://astro.uibk.ac.at/astroneu/hydroskiteam/index.htm
Otonyo Mangete
Affiliation:
Department for Mathematics and Statistics, University of Edinburgh JCMB, Mayfield Road, Edinburgh, EH9 3JZ, UK
Max Ruffert
Affiliation:
Department for Mathematics and Statistics, University of Edinburgh JCMB, Mayfield Road, Edinburgh, EH9 3JZ, UK
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Abstract

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We present first results of numerical simulations of the dynamics of all three components of a galaxy cluster: the dark matter, the intracluster gas, and the member galaxies. Our first aim is to understand the enrichment of the gas component by studying various interaction processes between cluster galaxies and the intracluster gas, notably ram-pressure stripping and galactic winds. Our second aim is to find out how fast metals originating from such interaction processes diffuse throughtout the cluster, in order to understand observed metallicity maps of galaxy clusters obtained from X-ray observations.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUC195 , March 2004 , pp. 285 - 289
Copyright
© 2004 International Astronomical Union