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Thorough characterisation of the 16 Cygni system. I. Forward seismic modelling with WhoSGlAd

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Figure

Fig. 2. Summary of 16 Cyg B best-t models. The colours are the same as in Fig. 1
Table 4. Adjusted stellar parameters including the T ef f con- con-straint and turbulent mixing with a coecient of D turb = 7500 cm 2 s −1 .
Fig. 7. Comparison of adjusted stellar parameters for both stars at a given physics. The straight line shows the locus of identical stellar parameters for both stars.
Table 6. Best individual models for each star, accounting for both seismic and non-seismic constraints.
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