Color-Magnitude Diagrams of Five Faint Clusters of the Large Magellanic Cloud

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Scientific paper

Color-magnitude diagrams of five faint clusters in the Large Magellanic Cloud are obtained by astrophotometry of ADH Schmidt plates centered on three faint photoelectric sequences. Two of the clusters are old, with well-established giant branches that are at least 2 mag brighter than their main sequences, while the other three are young, with bright, sparsely populated main sequences and several giant members.

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