Fig. 5
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Kiel diagram of stars listed in Table B.1. In the case of SB2 systems, parameters of the hotter component are displayed. Solid lines represent MESA evolutionary tracks for the stellar mass values M of (from right to left) 1.5, 3.0, 4.5, 7.0, and 13 M⊙ and a minimum amount of overshoot ƒOV = 0.005 Hp. The tracks are from Johnston et al. (2019b).
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