Carbon abundance at main sequence turn-off as a function of specific angular momentum of accreted material in models with rotational mixing only. To avoid excessive crowding, only models with M1 = 1.25 M⊙ are plotted, in which [C/H] ≃ 0.38 after mass transfer in all cases. The general result of little to no dilution for ja ≲ 2 × 1016 cm2s-1 holds for systems with other primary masses.
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