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Cluster Galaxy Evolution from a New Sample of Galaxy Clusters at 0.3 <z< 0.9
2001
Astrophysical Journal
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(Abridged) We analyze photometry and spectroscopy of a sample of 63 clusters at 0.3~ 5) and in which many of these galaxies, if not all, accrete mass either in the form of evolved stellar populations or gas that causes only a short term episode of star formation at lower redshifts (1.5 < z < 2). Our data are too crude to reach conclusions regarding the evolutionary state of any particular cluster or to investigate whether the morphological evolution of galaxies matches the simple scenario we
doi:10.1086/323942
fatcat:sjya4yijtnetdkllhf7h4jlas4