Fig. C.1.
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Timescale associated with the stellar rotational angular momentum as a function of system age for a twin system with high eccentricity (e = 0.55) and rapid initial rotation (Ωrot = 0.2Ωcrit), as presented in Fig. 5. The displayed modes are retrograde, with orbital harmonics k indicated by colour. Resonance locking occurs successively with modes of different orbital harmonics.
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