Fig. 4.
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Mass transfer rate cycle on our model for different irradiation efficiencies. Here, the mass of the companion star is 1.9 M⊙. The solid, dashed, and dotted lines represent irradiation efficiencies of 0.2, 0.6, and 1.0, respectively. Here, the Ṁst and Ṁcr represent the stable accretion rate and the critical accretion rate onto the WD, respective.
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