Fig. 4.
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Variation in [Fe/H] (solid lines) and [M/H] (dashed lines) from the ZAMS to the tip of the RGB for [Fe/H]i = 0.06. The purple and red lines represent models with and without turbulent mixing (both with radiative acceleration), and the cyan lines represent the model with only turbulent mixing. Top panel: is for the 1.2 M⊙ models and bottom panel: is for the 1.4 M⊙ models.
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