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Fig. 12.
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Comparison between the Georgy et al. (2013) (solid lines) and Lagarde et al. (2012) (dashed lines) evolutionary tracks with rotation at Z = 0.014 for M = 3 M⊙, 4 M⊙. Stars in the sample with M = 3.5 M⊙, 4 M⊙ and −0.1 < [Fe/H]< 0.1 are shown with error bars. The colour index indicates the [N/C] abundance ratios.
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