Fig. 8.

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Chemical structure of the mass fraction of hydrogen (red lines), helium (green lines), carbon (blue lines), and oxygen (purple lines) as a function of interior mass for the considered 10 M⊙ star. Panels E, F, G, and H correspond the evolutionary points labelled E, F, G, and H in Fig. 1, respectively. Left panels: for the 10 M⊙ stars with Z = 0.014 but with different initial rotational velocities, vini = 0 km s−1, 120 km s−1, and 350 km s−1. Right panels: for the 10 M⊙ stars with Z = 0.0008 but with different initial rotational velocities.
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