Top left: mixing coefficient profiles Dmix (full lines) as a function of normalized radius when varying the overshoot parameter fov in the 3 M⊙ reference model. Dashed vertical lines indicate convective core boundaries rcc, obtained from the Schwarzschild criterion (e.g., Kippenhahn et al. 2012). Top right: density ρ (dotted lines) and radial magnetic field component Br profile (at θ = 5°; full line) for the same stellar model. Dashed vertical lines indicate the same as on the left. Bottom row: same as Fig. 4, but varying fov.
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