Fig. 3
Position of the components in the system 41 Eri in the mass-radius diagram for inclinations in the range 28−50° with a step of 2°. The red lines are isotherms interpolated in the stellar models. With Teff = 12 750 K for the primary and Teff = 12 250 K for the secondary, we obtain an inclination of 33.7°. Open circles indicate the position of the secondary component.
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