Globular Clusters 47 TUC and NGC6752

Details Globular Clusters 47 TUC and NGC6752 Globular Clusters 47 TUC and NGC6752

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.3684k&link_type=abstract

HST Proposal ID #3684

Computer Science

Hst Proposal Id #3684

Scientific paper

This proposal is devoted completely to globular clusters. It studies the two clusters NGC104 (47 Tuc) and NGC6752 in B and V, down to below 24th magnitude. Fields at the center and at 1 and 3 core radii will allow determination of the luminosity function and its variation with radial position. This will in turn allow a determination of the degree of equipartition, which cannot be observed from the ground. At the same time the WFC will concentrate on a single field in each cluster in V and I, reaching a limit of about 26th magnitude, for the faint luminosity function at a radius of 6.5 arcmin. In addition, a far-UV image is taken of the center of NGC6752, to study the distribution of extremely blue objects.

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