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Evolution of galaxies in clusters

B. M. Poggianti
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Abstract

I summarize what is know about the evolution of galaxies in clusters from the observational point of view presenting results at high (z~1), intermediate (z~0.5) and low (z~0) redshifts. I comment on the comparison between observations and predictions of CDM models, highlighting the observational landmarks more relevant for this comparison, such as the establishment and evolution of the morphology-density relation, the Butcher-Oemler effect, the evolution of red galaxies/ellipticals, the star formation histories of galaxies in clusters, the downsizing effect and the history of mass assembly.

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B. M. Poggianti. 2005-03-09. Evolution of galaxies in clusters. https://arxiv.org/abs/astro-ph/0503218

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