Evolutionary tracks for the same stellar evolution models shown in Fig. 2, here plotted in the effective sHR diagram (solid lines), for which the Eddington-factor can be read off from the ordinate on the right. For comparison, the tracks from Fig. 2 are also copied into this diagram (dotted lines). The right ordinate scale is not valid for them. The labels give the initial masses for the tracks drawn as solid lines.
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