Estimated log g_evol 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 g_evol > log g(λ₁,D) and those where log g_evol < log g(λ₁,D). The evolutionary models used to infer stellar masses are those by Ekström et al. (2012) without rotation.