Structure of Globular Clusters: Cycle 1 Observations

Details Structure of Globular Clusters: Cycle 1 Observations Structure of Globular Clusters: Cycle 1 Observations

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.3218k&link_type=abstract

HST Proposal ID #3218

Physics

Hst Proposal Id #3218

Scientific paper

NGC 6624 is a collapsed-core globular cluster with an X-ray source near its center. At ground-based resolution its core profile is unresolved. B and V exposures with the FOC should reach far enough down the main sequence to distinguish stars of different mass. The three FOC fields are the center and two neighboring regions. Simultaneous exposures are made in V and I with the WFC, to gain further structural information. These will go much deeper, since the orientations are arranged so as to keep the WFC on the same field at all times.

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