The Stellar Density Distributions in the Centers of Galactic Globular Clusters II. Cycle 0 Major Changes

Details The Stellar Density Distributions in the Centers of Galactic Globular Clusters II. Cycle 0 Major Changes The Stellar Density Distributions in the Centers of Galactic Globular Clusters II. Cycle 0 Major Changes

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.3111b&link_type=abstract

HST Proposal ID #3111

Physics

Hst Proposal Id #3111

Scientific paper

Short exposures will be made of all galactic globular clusters with distance moduli less than 15.5 mag and galactic latitude above or below 15 degrees. A search will be made for cusps in the stellar density distributions and the colors will be measured for the brightest stars in the cores of the clusters. ST observations are required in order to reach the innermost regions of the clusters with sufficient resolution to separate individual stars.

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