Fig. 5.
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Inertial dips overplotted for different core Lehnert number for a fixed envelope Lehnert number Leenv = 10−3 and coupling parameter ϵ = 1.5 × 10−2, in a uniformly rotating star, in the framework of a continuous N at ra. The dots are obtained by solving Eq. (82), and the continuous line by applying the dip profile given by Eq. (86).
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