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Fig. 8.

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Average frequency shift of the dipole modes caused by various internal magnetic field configurations as a function of the magnetic field strength for three stellar models. The field strengths have been chosen such that Bcen = 0.7 Bcrit, cen and BH = 0.7 Bcrit, H. The critical field strengths were calculated at ω = 2πνmax with l = 1. Colors correspond to different stellar models and symbols indicate that a different magnetic field configuration has been used. Average frequency shifts corresponding to the azimuthal order m = 0 (m = ±1) are shown as solid symbols (outlines). The field configurations and the calculation of the average frequency shifts are described in Sect. 4.3 and in the notes under Table 3, which also summarizes the data shown in this figure. Note that the horizontal axis is broken.

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