Fig. 5.
Angular velocity profiles vs the radius at solar age for models presented in Fig. 3 compared to the rotation profile of the Sun (in dark grey) obtained from helioseismology from Eff-Darwich et al. (2008). The solid line, the dotted line, the dashed line, and the dot-dashed line refer to the differential, solid, νadd, and νadd(t) rotation cases, respectively.
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