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Fig. 6

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Etot(V − I) vs. Wenv(Hα), for LMC (squares), Milky Way stars (triangles). Crosses belong to the SMC data of Coe et al. (2005) and spectral types from McBride et al. (2008). The line represents the relationship for LMC stars only. Some stars have error bars of the order of the the symbol size.

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