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Fig. 7


N/C and N/O ratios obtained from our spectral analysis. Squares and circles stand for the components of HD 17505Aa and HD 206267Aa, respectively. The filled (resp. empty) symbols correspondto the primary (resp. secondary) star. The coloured tracks show the predictions from solar metallicitysingle star evolutionary models of different initial masses. The left panel illustrates the comparison with models of Ekström et al. (2012) without rotation, whereas the tracks in the middle panel correspond to the models of the same authors but assuming an initial rotational velocity of 0.4 × vcrit. The right panel shows the comparison with the models of Brott et al. (2011) accounting for rotation. In the right panel, initial rotational velocities are 111, 110, 109, and 213 km s−1 for the 20, 25, 30, and 50 M models, respectively.

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