The impact of mass loss on the evolution of the depth (in temperature and mass) of the SCZ in 0.8 M⊙ models with atomic diffusion only, and with mass loss rates from 10-15 M⊙ yr-1 to 10-12 M⊙ yr-1. Upper row: HR diagram and the He and Fe surface abundances. Lower row: zoom on the Teff, and on the mass and temperature at the bottom of the SCZ.
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