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Fig. 7.

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HR diagram showing the evolution of a representative conservative MESA mass transfer model, with initial masses of 1.23 M (donor, orange) and 1.07 M (accretor, blue), and initial orbital period of 0.95 days. Filled squares mark the observed positions of S1082 Aa and Ab. Circles show the model positions at 4 Gyr, crosses indicate when mass transfer begins, and diamonds mark the positions at 4.87 Gyr after mass transfer has altered both stars’ evolution.

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