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Fig. 11.

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Probability density distribution of several properties of our binary models after Case AB mass transfer, when the central helium mass fraction of the donor has decreased to 0.90: orbital period versus mass ratio (top left), surface helium abundance and mass of the mass gainer (top right), leftover hydrogen mass in the donor and donor mass (bottom left), and surface nitrogen mass fraction enhancement versus rotational velocity of the mass gainer (bottom right).

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