Interactions and the Evolution of Cluster Galaxies

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

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.

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