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Fig. 2


Upper row: radiative accelerations for five atomic species, after 232 Myr of evolution in a model with a mass loss rate of 10-13   M/yr (red curves) and in a model with turbulence (blue curves). The dotted lines represent gravity. Lower row: corresponding mass fraction in the model with mass loss and in that with turbulence. The dashed lines are the original values, which correspond to an original metallicity of Z0 = 0.01.

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