Fig. 8.
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Left panel: change in the convection zone mass over the evolutionary time from the onset of the helium flash for the 1.3 M⊙ solar metallicity stars with different initial rotational velocities. Right panel: lithium abundance as a function of evolutionary time from the onset of the helium flash for the 1.3 M⊙ solar metallicity stars with different initial rotational velocities.
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