Fig. 4.
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Core rotation rates as a function of the surface gravity for 1.1 M⊙ models of sub-giant and red giant stars computed with the MESA code. The red and blue lines correspond to the revised version of the dynamo by Fuller et al. (2019) (i.e., n = 3 and CT = 1) and the asteroseismic-calibrated version of the TS dynamo (n = 1 and CT = 216), respectively.
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