Fig. 8.
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Evolution of the convective core mass during the main sequence for the 3 M⊙ (left panel) and 60 M⊙ (right panel) models at different metallicities (Z = 0 (Pop III, blue), Z = 10−5 (this paper, green), Z = 0.0004 (I Zw 18, yellow), Z = 0.006 (LMC, pink), and Z = 0.014 (solar, purple)). Solid lines: Non-rotating models. Dotted lines: Rotating models.
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