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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