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Fig. B.1


Radiative accelerations after 232 Myr evolution in a model with mass loss of 10-13   M/yr (red curves) and in a model with turbulence with ΔM0 = 1.4  ×  10-6   M (blue curves) for all calculated atomic species. The sharp mimima in the grad(Ti), grad(Cr), and grad(Mn) curves at log ΔM/M ~  − 10 appear surprising but have been verified to be a systematic property of the OPAL atomic data.

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