Fig. E.1.

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Top panel: Rotation rate (logarithmic scale) as a function of the fractional stellar mass. The line colour represents the evolutionary stage of the model in terms of mixed mode density. The dashed lines represent models computed using MESA angular momentum transport prescription. The solid lines represent models computed using our angular momentum transport prescription. The left, centre and right panels showcase models with different stellar masses. Bottom panel: Relative difference in rotation rate between MESA and our models.
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