Fig. 7.
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r010 ratios according to the frequency for a M = 1.40 M⊙ model at XC = 0.10 for different values of relative-to-the-Sun magnetic field values Brel. We set i = 0° and [λmin; λmax]=[11; 53]. The blue, orange, and green points corresponding to Brel = 0, 1, and 1.2, respectively, are almost completely overlapping because the shift induced by the magnetic field is small.
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