Cooling Flows in Distant Clusters - Cycle 2

Details Cooling Flows in Distant Clusters - Cycle 2 Cooling Flows in Distant Clusters - Cycle 2

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.3487m&link_type=abstract

HST Proposal ID #3487

Physics

Hst Proposal Id #3487

Scientific paper

Cooling flow galaxies will be imaged in the light of the emission line
[OII]3727 and neighbouring blue/UV continuum. The observations will
enable us to locate regions of ongoing star formation, image the
emission filaments at high spatial resolution and determine if they are
dusty.

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