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Fig. 3

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Scaled contributions to the splittings due to the implicit third-order terms in the eigenfrequencies , the Coriolis effect , distorsion , the coupling of the two , and near degeneracy. Left: for  = 1 g-modes. Right: for  = 1 p-modes, divided by the square of the central frequency. 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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