UBVRI Photometry of the Globular Cluster NGC 6752

Details UBVRI Photometry of the Globular Cluster NGC 6752 UBVRI Photometry of the Globular Cluster NGC 6752

Feb 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000noao.prop..384c&link_type=abstract

NOAO Proposal ID #2000A-0384

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Scientific paper

We propose using the 0.9-m telescope to obtain UBVRI CCD photometry of the globular cluster NGC 6752. Modern data regarding the photometry of this nearby cluster are severely lacking for this basic filter system. By carrying out this program we will provide important detailed information regarding the characteristic of this cluster's color-magnitude diagram (CMD). CMD's are important diagnostics of such things as cluster age, distance, stellar luminosity functions and cluster metallicity, which in turn constrain stellar evolution models, Galactic formation scenarios and cosmological models.

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