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The distance to NGC 6397 by M-subdwarf main-sequence fitting

ASTRONOMICAL JOURNAL, no. 6 (1998): 2929-2935

Cited by: 62|Views7

Abstract

Recent years have seen a substantial improvement both in photometry of low-luminosity stars in globular clusters and in modeling the stellar atmospheres of late-type dwarfs. We build on these observational and theoretical advances in undertaking the first determination of the distance to a globular cluster by main-sequence fitting using s...More

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