BVI Photometry and the Luminosity Function of M92

Details BVI Photometry and the Luminosity Function of M92 BVI Photometry and the Luminosity Function of M92

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.5210p&link_type=abstract

American Astronomical Society Meeting 203, #52.10; Bulletin of the American Astronomical Society, Vol. 35, p.1290

Astronomy and Astrophysics

Astronomy

Scientific paper

We present BVI observations of the Galactic globular cluster M92 obtained with the 2.4m Hiltner telescope at the MDM Observatory. The observations were conducted under good seeing conditions and cover a region 34 arcminutes square. Accurate photometry is presented for over 23,000 stars including nearly 4000 stars brighter than the main sequence turn-off. We also present luminosity functions derived from the ground-based data and Hubble Space Telescope observations and compare them with theoretical models.

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