Fig. A.1.
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Orbital changes as a function of the donor mass due to the wind accretion processes with M1, i = 3.41 M⊙, M2, i = 3.06 M⊙. The grey line is for af/ai ≃ 0.71, corresponding to the peaks of P1, mt/Pi distributions in Figure 4. The results for βW from 0.5 to 1 are shown in black and red lines, as marked in the plot. We note that the wind accretion efficiency is equal to 1 − βW.
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