N-body/SPH study of the evolution of dwarf galaxies in a cluster environment

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dc.creatorMichielsen, Dolf
dc.creatorDe Rijcke, Sven
dc.creatorDejonghe, Herwig
dc.date2004-11-19
dc.date.accessioned2026-07-07T02:15:57Z
dc.date.available2026-07-07T02:15:57Z
dc.descriptionUsing an N-body/SPH code, we explore the scenario in which a dwarf elliptical galaxy (dE) is subjected to ram-pressure stripping due to the intracluster medium (ICM). Our simulations show that while (i) smaller dEs lose their ISM almost immediately after entering the cluster, (ii) more massive dEs are able to retain their gas for considerable timespans.
dc.description1 page, no figures, poster contribution to the Splinter Meeting "Galaxies in interaction" at the joint meeting of the Czech Astronomical Society and the Astronomische Gesellschaft (20-25 Sept. 2004, Prague, Czech Republic)
dc.identifierhttps://arxiv.org/abs/astro-ph/0411576
dc.identifierhttp://arxiv.org/abs/astro-ph/0411576
dc.identifierAstron.Nachr. 325S1 (2004) 122
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8606
dc.subjectAstrophysics
dc.titleN-body/SPH study of the evolution of dwarf galaxies in a cluster environment
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