High Precision Photometry of the Core of M13

Details High Precision Photometry of the Core of M13 High Precision Photometry of the Core of M13

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999hst..prop.8278b&link_type=abstract

HST Proposal ID #8278

Physics

Hst Proposal Id #8278 Stellar Populations In Clusters

Scientific paper

We propose to obtain highly precise main sequence photometry in V and I in the core of the globular cluster M13. The data will be used to search for a binary sequence, and to obtain highly accurate main sequence ridge lines and a deep luminosity function in the core regions of the cluster. The dynamics and horizontal branch morphology of M13 are anomalous, and it seems likely than an understanding of the core binary population will be required to resolve the problems they raise.

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