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Fig. 4

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Position of the program stars in a (Teff,log (g)) diagram. Overlaid are evolution tracks for non-rotating stars (Ω / Ωcrit = 0) of metallicity Z = 0.014 and different initial masses (M ≤ 15 M: Georgy et al. 2013; otherwise: Ekström et al. 2012). Black filled circles and numbers mark the age in Myr. Red numbers correspond to those of Table 4. Error bars indicate 99%-confidence limits.

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