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Fig. 4


Behavior of left: the scaled integrals β and γ (Eq. (27)), right: the scaled contributions to the splitting, as a function of the radial order n (Eqs. (31) to (33)). Computations were made for an 8.5 M ZAMS model uniformly rotating at 15%   Ωk, i.e. 95   km   s-1 (see stellar parameters in Table 1).

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