Main sequence of NGC 6171 (Ferraro+, 1995)

Physics

Scientific paper

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Clusters: Globular, Photometry

Scientific paper

Deep J, K IR-array photometry for individual Main Sequence stars in NGC 6171 reaching K~18, about two magnitudes below the turnoff, is presented. The observations were made during 3 nights on June 1993 at the 2.2m ESO/MPI telescope at ESO (La Silla), equipped with the IR-array camera IRAC2.
(1 data file).

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