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Fig. 13
Distribution of the ratio v/vcrit of true rotational velocities as a function of the fractional age in the MS evolutionary phase for normal stars in the mass interval 1.7 ≤ M ≤ 3.3 M⊙. The filled circles are the average positions of the stars in running boxes with bins of 0.15 in t/tMS and 0.5 in M/M⊙.
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