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Fig. 19.

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Hertzsprung-Russell diagram: evolutionary tracks of Clés models for the secondary star of Minit = 7.5 M (water green), 7.7 M (dark blue), and 8.0 M (orange), and DT = 0 cm2 s−1 (solid line), 2 × 105 cm2 s−1 (dashed line), and 5 × 105 cm2 s−1 (dotted-dashed line). All models have αov = 0.30 and ξ = 0.1. The filled 5-branch stars over-plotted on the tracks correspond to the models for which the age is equal to the age of the best-fit models of the primary star (i.e. about 9 Myr). The observational value is represented by the red point, and its error bars are represented by the dark red parallelogram.

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