Fig. 7.
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Evolutionary tracks of 0.8, 1.0, 1.5, 2.0, and 2.5 M⊙ stars calculated with the MLT (mixing length parameter Λ = 1.68) indicated by crosses and the SFCT indicated by the solid lines of different colors. The comparison shows that the SFCT with no mixing length parameter is equivalent to the classical MLT with calibrated mixing length parameter. Data are from Pasetto et al. (2016).
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