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The Evolution of Galaxies in Clusters

Published online by Cambridge University Press:  26 May 2016

John Dubinski ,
Dan Koranyi  and
Margaret Geller
John Dubinski
Affiliation:
Department of Astronomy and Astrophysics/CITA, McLennan Labs, 60 St. George St., University of Toronto, Toronto, ON, Canada M5S 3H8
Dan Koranyi
Affiliation:
Harvard-Smithsonian Centre for Astrophysics, 60 Garden St., Cambridge, MA, USA 02138
Margaret Geller
Affiliation:
Harvard-Smithsonian Centre for Astrophysics, 60 Garden St., Cambridge, MA, USA 02138

Abstract

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We report on recent numerical investigations of the dynamical evolution of galaxies in clusters. Simulations of spiral galaxies falling into forming clusters show the development of the morphology-density relationship and the formation of regular and giant elliptical galaxies. The regular elliptical merger remnants end up in a fundamental plane very similar to the observed relation. The giant ellipticals have much in common with their real counterparts but their central velocity dispersions are too high. We also quantify the amount and distribution of diffuse light in clusters.

Information

Type
Cosmology
Information
Symposium - International Astronomical Union , Volume 208: Astrophysical Supercomputing using Particle Simulations , 2003 , pp. 237 - 244
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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