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 ℓ = 1 g-modes. Right: for ℓ = 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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