Fig. 14
Radius and gravity associated with atmosphere models (full line) and evolutionary models (dashed line). The shaded area corresponds to the uncertainty on the radius of the atmosphere models to match the absolute flux of HD 206893B. We used the ExoREM atmosphere models, which provide the best fit to HD 206893B (see Sect. 5.3), and the Baraffe et al. (2003) evolutionary models.
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