Fig. 20
HR diagram showing where the stellar sequences of three different grids begin the main-sequence evolution (ZAMS, marked with black dashed lines) and where they finish the main-sequence evolution (TAMS, shaded regions). G+13: Georgy et al. (2013); MM02: Meynet & Maeder (2002); the initial metallicity of the grids is also indicated by the legend.
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