Fig. 7
Location of the primary component of HD 165246 in Teff vs. log g plane. Evolutionary tracks for models are labelled by their mass in the solar units. Evolutionary models by Brott et al. (2011) for the initial rotational velocities of v = 0 and 270 km s-1 are plotted as solid and dotted lines, respectively. Isochrones are plotted as solid and dotted thin lines.
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