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Fig. 4.

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Mass-transfer rate (upper panel) and BH spin χBH (lower panel) as functions of the model number. The dashed line indicates the standard Eddington accretion rate (1.0 ̇MEdd). In the binary sequence shown, the initial masses of the BH and He-rich star are 3.6 M and 6.0 M, respectively, with an initial orbital period of 0.08 days. Different MT phases are highlighted in various colors: Case BA (green), case BB (blue), and case BC (gray).

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