Oscillations of red giant stars with magnetic damping in the core - I. Dissipation of mode energy in dipole-like magnetic fields

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Fig. B.4.

Same as Fig. 6, now considering the strength of the radial component of the internal magnetic field at the hydrogen-burning shell. Here, we consider the ratio B_H / B_crit, H instead of B_cen / B_crit, cen when using Eq. 13.

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