Galaxy properties in a Filament in Abell 851

Details Galaxy properties in a Filament in Abell 851 Galaxy properties in a Filament in Abell 851

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006hst..prop10820d&link_type=abstract

HST Proposal ID #10820. Cycle 15

Physics

Scientific paper

We propose to image two fields that cover the filament of galaxies that is streaming into the remarkable cluster Abell 851, z=0.41, one of the two examples of the expected mechanism of cluster growth. These observations will test theories of alteration of galaxy morphology and star formation history for galaxies infalling into intermediate redshift clusters.

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