Enrichment of the intracluster medium from infalling galaxies

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...

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Veröffentlicht in:Proceedings of the International Astronomical Union 2004-03, Vol.2004 (IAUC195), p.285-289
Hauptverfasser: van Kampen, Eelco, Domainko, Wilfried, Kapferer, Wolfgang, Schindler, Sabine, Kimeswenger, Stefan, Mangete, Otonyo, Ruffert, Max
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container_end_page 289
container_issue IAUC195
container_start_page 285
container_title Proceedings of the International Astronomical Union
container_volume 2004
creator van Kampen, Eelco
Domainko, Wilfried
Kapferer, Wolfgang
Schindler, Sabine
Kimeswenger, Stefan
Mangete, Otonyo
Ruffert, Max
description 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
doi_str_mv 10.1017/S1743921304000602
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source Cambridge University Press Journals Complete
subjects Astronomy
Contributed Papers
title Enrichment of the intracluster medium from infalling galaxies
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