Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators? - Implications for measurements of rotation and internal magnetic fields

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Fig. 9.

Same as Fig. 6 but for a model with X_c ≈ 0.4. The fraction of critical rotation of this model is 0.0942 Ω_c, Kep. Black symbols corresponds to ℓ = 1, red symbols to ℓ = 2. For comparison, the results from the ZAMS model at 0.1 Ω_c, Kep from Fig. 6 are also shown in blue.

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