Fig. 2.

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Evolution of the total mass, the convective core mass, and the helium core of the donor model with an initial mass of 20 M⊙ with a companion of initially 14 M⊙ and an initial orbital period of 100.35 d = 2.2 d (top panels) and 100.75 d = 5.6 d (bottom panels). We indicate the mass of the convective core at the onset of mass transfer, just after the fast Case A, and at central hydrogen depletion by grey lines.
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