Interactions and the Evolution of Cluster Galaxies |
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| Authors: | R Vílchez-Gómex G A Bruzual R Pelló R Domínguez |
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| Institution: | (1) Escuela Politécnica, Avda. de la Universidad, s/n, 10071 Cáceres, Spain;(2) Centro de Investigaciones de Astronomía, Apartado Postal 264, Mérida, 5101-A, Venezuela;(3) Observatoire Midi-Pyrénées, 14 Av. Edouard Belin, F-31400 Toulouse, France;(4) Departament d'Astronomia i Meteorologia, Martí i Franquès 1, 08028 Barcelona, Spain |
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| Abstract: | We have developed model predictions for the morphological distribution of cluster galaxies as a function of the cluster-centric
distance and the local galaxy density, using a semi-analytical code. This code allows us to obtain magnitudes and colours
for cluster galaxies at different redshifts, and thus to study in detail the evolution of the colour–magnitude relation of
specific distant clusters.
This revised version was published online in July 2006 with corrections to the Cover Date. |
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