History of Mass Assembly and Star Formation in Galaxy Cluster

Computer Science

Scientific paper

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Scientific paper

We will ask a fundamental question: ie, how the star formation is truncated in cluster environment in the course of hierarchical assembly of dark matter haloes. This is the central question of the Butcher-Oemler effect and the environmental effect seen in local and distant clusters. We try to answer this fundamental question by comparing the galaxy properties in detail as a function of time (redshift) and the environment using the CNOC clusters data and our own Subaru wide-field data of distant clusters. We derive the global star formation history in clusters by sketching the flow of galaxies across the colour-magnitude plane over a large fraction of the Hubble time, and connect this to the large scale structure of clusters traced by the photometric redshift technique.

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