Fig. 2.

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Example of the evolution of a binary. The solid line, dashed line, and dash-dot line represent the mass of the WD (MWD), the mass of the companion star (M2), and the mass transfer rate between the binary (ṁ), respectively. The initial mass of the WD is 1.25 M⊙, and the mass of the companion star is 2.0 M⊙. The initial binary orbital period is 1.7 d. Here, the Ṁst represents the stable accretion rate onto the WD.
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