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Fig. 14.


γ index as a function of Teff for WTTSp (upper panels) and CTTSe (lower panels) cluster members split into two different age ranges. The solid lines indicate the best fits obtained from a second order polynomial fit of the data while the dashed line indicates the reference locus of MS stars obtained in Damiani et al. (2014). The dotted lines indicate the polynomial fit at 3σ.

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