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Fig. 1


Sketch of the stellar structure studied here. We consider a two-layered star: a radiative core of rotation rate Ωrad and a convective envelope of rotation rate Ωconv. Both are assumed to rotate as a solid body with different rotation rates. In red we indicate the different processes included in the model. The convective envelope is subjected to external torques (stellar wind and tidal torques), as well as torques due to the radiative core development and coupling with the convective envelope.

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