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• W3100651627 abstract "We present {it Hubble Space Telescope} {it V,I} photometry of the central region of the LMC cluster NGC 1866, reaching magnitudes as faint as V=27 mag. 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 {it global} cluster luminosity function as obtained from stars in all 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." @default.
• W3100651627 created "2020-11-23" @default.
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• W3100651627 date "2003-06-01" @default.
• W3100651627 modified "2023-09-25" @default.
• W3100651627 title "The Luminosity Function of the Large Magellanic Cloud Globular Cluster NGC 1866" @default.
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• W3100651627 doi "https://doi.org/10.1086/374946" @default.
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