Fig. 3 from Distances to Populous Clusters in the Large Magellanic Cloud via the K‐band Luminosity of the Red Clump

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Distances to Populous Clusters in the Large Magellanic Cloud via the K‐band Luminosity of the Red Clump

Authors: Aaron J. Grocholski, Ata Sarajedini, Knut A. G. Olsen, Glenn P. Tiede, and Conor L. Mancone

Grocholski et al. 2007 The Astronomical Journal 134 680.

Provider: AAS Journals

Caption: Fig. 3.

Near‐infrared CMDs for the 17 clusters in our sample. Cluster RCs are denoted by the box, and all stars within this box are used in calculating ﹩M^{\mathrm{RC}\,}_{K}﹩.

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