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Chapter
Recent Star Formation in Very Luminous Infrared Galaxies
Among star forming galaxies, a spectral combination of a strong Hδ line in absorption and a moderate [OII] emission has been suggested to be a useful method to identify dusty starburst galaxies at any redshift...
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Chapter
Evolution of Galaxy Morphologies in Clusters
We have studied the evolution of galaxian morphologies from ground-based, good-seeing images of 9 clusters at z=0.09−0.25. The comparison of our data with those relative to higher redshift clusters (Dressler et a...
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Article
Evolution of Galaxy morphologies in Clusters
We have studied the evolution of galaxian morphologies from ground-based, good-seeing images of 9 clusters at z=0.09-0.25. The comparison of our data with those relative to higher redshift clusters(Dressler et al...