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Fig. 2.

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Accreted mass (the color bar) as a function of the initial orbital period and initial mass of He-rich stars. Cross: Initial Overflow; square: Case BA; triangle: Case BB; diamond: Case BC); circle: No mass transfer (MT). Left panel: high-spin prior (NS mass m1 = 2.02 M), right panel: low-spin prior (NS mass m1 = 1.74 M). We mark the parameter space of Case BB and Case BC with light and dark grey backgrounds, respectively.

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