Fig. B.3.
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Boron abundances as a function of log g for 15 M⊙vini/vcrit = 0.4 magnetic models computed with the asteroseismic-calibrated prescription for the transport by the Tayler instability of Eggenberger et al. (2022) (straight blue line), the prescription of Fuller et al. (2019) (dashed orange line) and the one of Spruit (2002) (dotted red line).
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