Fig. 4.
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Mass of the convective core (in the unit of the whole stellar mass) as a function of evolutionary age. Panel a: for the 10 M⊙ stars with Z = 0.014 but with different initial rotational velocities of vini = 0 km s−1, 120 km s−1, 250 km s−1, 350 km s−1. Panel b: for the 10 M⊙ stars with Z = 0.0008 but with the corresponding different initial rotational velocities.
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