Fig. 1
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Stellar wind rates for low mass donors with initial masses M1 = 1.7 M⊙ (left) and 3.0 M⊙ (right), calculated using MESA. The first peak of the stellar wind corresponds to the red giant branch (RGB) stage. The second peak associated with the envelope loss by the star corresponds to the stage of the AGB. The zero moment of time t = tZAMS = 0 corresponds to the ZAMS.
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