Fig. 3.

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Central (solid) and surface (dashed) abundances as a function of time of a 240 M⊙ star for Z = 10−11 (left), Z = 0.001 (center), and Z = 0.014(right). The abscissa is the time until the last model, and the ordinate is the mass fraction of each element. Light blue, light green, pink, dark blue, purple, dark green, and orange refer to H, 4He, 12C, 14N, 16O, 20Ne + 22Ne, and 24Mg + 25Mg + 26Mg abundances, respectively. Colored bars at the top indicate the type (H, He, and C) and duration of core burning phases. The red square marks the time when XHS < 0.3 in mass fraction.
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