Fig. 2.

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Evolution of 19F at the surface (Fs) and at the centre (Fc) of a 120 M⊙ star for different metallicities and rotations, as indicated in each panel (in arbitrary units). The evolution of the total mass (Mtot) and the mass of the convective core (Mcc) are also shown. The gray dashed lines indicate the end of the core H-burning phases. The upper panels show models at LMC metallicity, while the lower panels show models at solar metallicity.
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