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Fig. 1.

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Radiative accelerations for Sc vs. log T at the beginning of the MS for a chemically homogeneous 1.5, 1.7, and 2 M model (red, black, and blue sets of curves, respectively). For each mass, the short-dashed, long-dashed, and dash-dotted curves show the grad for an abundance one-tenth, ten times, and a hundred times the solar value respectively. The dotted curves denote the local gravity.

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