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Fig. 14

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Comparison of evolutionary tracks calculated by Ekström et al. (2012), with and witout rotation, and those of Bertelli et al. (2009). Systematic differences could appear in the determination of stellar masses and ages when one or the other series of evolutionary models are used. They are not significant compared to those that can still arise from rotational effects once the apparent fundamental parameters are consistently treated for the rotational effects.

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