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Fig. 13


Estimated log gevol parameters with models of stellar evolution against log g(λ1,D) obtained with the BCD calibrations. As in Fig. 12, circles denote stars in NGC 3766, while squares denote stars in NGC 4755. We also indicate the marked stellar masses and radii for which log gevol > log g(λ1,D) and those where log gevol < log g(λ1,D). The evolutionary models used to infer stellar masses are those by Ekström et al. (2012) without rotation.

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