The Luminosity Function of the Large Magellanic Cloud Globular Cluster NGC 1866

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© 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation E. Brocato et al 2003 AJ 125 3111 DOI 10.1086/374946

1538-3881/125/6/3111

Abstract

We present Hubble Space Telescope VI photometry of the central region of the Large Magellanic Cloud cluster NGC 1866, reaching magnitudes as faint as V = 27. We find evidence that the cluster luminosity function shows a strong dependence on the distance from the cluster center, with a clear deficiency of low-luminosity stars in the inner region. We discuss a global cluster luminosity function as obtained from stars from all parts of the investigated region, which appears in impressive agreement with the prediction from a Salpeter mass distribution. We also revisit the use of NGC 1866 as a probe for determining the efficiency of core overshooting and conclude that a definitive answer to this question is not possible from this cluster.

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10.1086/374946