ar X iv : a st ro - p h / 97 09 05 5 v 1 6 S ep 1 99 7

Abstract

We identify a vertical extension of the red clump stars in the color magnitude diagram (CMD) of a section of the Large Magellanic Cloud (LMC). The distribution of stars in this extension is indistinguishable in the U , B, V , and I bands — confirming that the detection is real and placing a strong constraint on models of this stellar population. After… (More)

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Cite this paper

@inproceedings{Lin1997arXI, title={ar X iv : a st ro - p h / 97 09 05 5 v 1 6 S ep 1 99 7}, author={Douglas N. C. Lin}, year={1997} }