Paper:	Disk Galaxies in Distant Clusters
Volume:	230, Galaxy Disks and Disk Galaxies
Page:	613
Authors:	Poggianti, B. M.
Abstract:	Disk galaxies in clusters (spirals and S0's) have gone through important transformations during the past few Gyr. In fact, while the ellipticals in dense regions seem to have changed little since at least z=0.5, both the morphology and the star formation activity of the disk galaxies have evolved significantly. Here we present the results of the first morphological study of galaxies in clusters at z=0.1-0.25 (Fasano et al. 2000), showing the evolution of the morphological fractions and of the morphology-density relation.

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