Notes. i denotes the inclination of the spin axis with respect to the sky plane; m, mass; Ω, the orientation of star’s equator, as seen by the observer; R_equiv, equivalent radius; θ_equiv, angular diameter; P_rot, rotational period; v, circumference velocity. Except for the temperature T, all the parameters were determined from interferometry. The values of χ_VIS² do not exhibit a significant minimum, because the model is too constrained by v sin i. Then, we kept the determined parameters fixed and fitted the temperature according to the spectroscopic data to find χ_SPE². However, synthetic line profiles were in all cases deeper than the observed ones. The model with the lowest χ_VIS² and χ_SPE² is for i = 14 deg. For models based on interferometry, the parameters i, log g = 3.0, v sin i = 70 km s⁻¹, T = 25 000 K were fixed, while m, Ω were free.