Star Formation Rates in Distant Cluster Galaxies: Cycle 4 Carry-Over

Details Star Formation Rates in Distant Cluster Galaxies: Cycle 4 Carry-Over Star Formation Rates in Distant Cluster Galaxies: Cycle 4 Carry-Over

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5709d&link_type=abstract

HST Proposal ID #5709

Computer Science

Hst Proposal Id #5709 Galaxies &Amp, Clusters Evolution/Cosmology

Scientific paper

Multicolor photometry and spectroscopic redshifts are available for a complete sample of faint galaxies in the southern cluster Abell 370 at a redshift of z=0.37. Strong evidence has been found for residual star formation in the red cluster galaxies. This may reflect general evolution in the cluster ellipticals, or it could represent the final transition from infalling gas-rich systems to present-day lenticular galaxies. WFPC2 will be used to extend the spectral energy distributions for cluster members into the UV providing direct measures of the proportions of young and evolved stars in a carefully selected sample of red members complete to K=17.0.

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