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Fig. 7.
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Same as Fig. 5 for NGC 2451 B (top) and NGC 2547 (bottom). In this case, the best-fit model (solid blue line) corresponds to αML = 2.0 and βspot = 0. The long-dashed green line shows the isochrone with the same age, reddening, and αML as the best-fit model, but computed with βspot = 0.2.
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