Fig. 10.
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Evolutionary tracks across the spectroscopic Hertzsprung-Russell diagram (Langer & Kudritzki 2014) for model stars without rotation, calculated for self-consistent tracks (solid lines) and for classical tracks (dashed lines). Grey shaded area represents the region where self-consistent m-CAK prescription is valid (Teff ≥ 30, log g ≥ 3.2, see Gormaz-Matamala et al. 2022). Black dots represent the same as indicated in Fig. 6.
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