Fig. 8.
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Binary evolution of J1710 from the present day until the sdB star evolves into a WD, modeled using the MESA code. In the top two panels, the moment when the sdB phase ends is marked with a star. In each subplot, the green lines correspond to the left vertical axis, and the red lines correspond to the right vertical axis. Detailed descriptions of the panels are provided in Sect. 4.2.
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