Fig. 5
Evolution of six key parameters as a function of the donor-star age from the zero-age main sequence for an IMXB with a donor-star mass of 2 M⊙ and an initial period of 1.4 days. Top left panel: donor-star mass. Middle left panel: center He abundance. Bottom left panel: mass-transfer rate. Top right panel: mass fraction of the convective envelope. Middle right panel: orbital period. Bottom right panel: donor-star radius.
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