Fig. 11
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Convective turnover timescale as a function of stellar age. The black circles show the stars studied in this work while the continuous lines represents the tracks provided by Spada et al. (2013). The models have solar metallicities and stellar masses ranging from 0.10 M⊙ to 1.25 M⊙ (from red to violet) with a mass step of 0.05 M⊙
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