Fig. 4 from Infrared Photometry of Red Supergiants in Young Clusters in the Magellanic Clouds

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Infrared Photometry of Red Supergiants in Young Clusters in the Magellanic Clouds

Keller 1999 The Astronomical Journal 118 889.

Caption: Fig. 4.

H‐R diagram showing evolutionary tracks from the models of the Geneva group for Z = 0.004 (dotted lines) at 10 and 4 M_⊙. Symbols are as in Fig. 3.