The Stellar Density Distribution in the Center of the Galactic Globular Cluster M15

Details The Stellar Density Distribution in the Center of the Galactic Globular Cluster M15 The Stellar Density Distribution in the Center of the Galactic Globular Cluster M15

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.3040b&link_type=abstract

HST Proposal ID #3040

Physics

Hst Proposal Id #3040

Scientific paper

Short exposures in the V and I bands will be made of the Galactic globular cluster M15 with the Planetary Camera. These exposures will be an important test of the ability of the HST to do crowded field photometry. Simulations suggest that the HST observations will be much more powerful than ground-based observations and can provide a useful constraint on a central Massive Black Hole.

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