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Fig. 7.

Fig. 7. Refer to the following caption and surrounding text.

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Upper panel: Same as Figure 3, but for a binary with a 20 M BH companion. The solid (dashed) lines denote models with (without) the TS dynamo. The lines in different colors correspond to the various He stars initial rotation rates (blue: ωi = 0; orange: initially synchronized with the orbit; green: ωi = 0.3 ωcrit; red: ωi = 0.6 ωcrit; purple: ωi = 0.9 ωcrit). Lower panel: Total internal angular momentum as a function of mass coordinate within the corresponding models at carbon depletion.

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