Galaxy evolution in a large sample of X-ray clusters
The evolution of galaxy populations is dependent upon the environment in which they are located, from low mass galaxy groups to rich galaxy clusters. However, what remains unclear is which physical process(es) dominate this evolution. We investigate this using uniform CFHT Megacam photometry for X...
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Language: | English en |
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2013
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Online Access: | http://hdl.handle.net/1828/5089 |