Notes. In some cases more values are listed for a parameter, to show that the methods do not contradict each other. Because they were safely resolved only with the astrometry, elements of orbit 3 are not listed here, but in Table 10 and the mass of component C is estimated and briefly discussed in Sect. 7. The listed parameters are the anomalistic period P_AN, the sidereal period P_S, the periastron epoch T_p, the epoch of the primary minimum T_min, the semi-major axis a, the mass ratio q, the eccentricity e, the inclination i, the periastron argument ω, the position angle of the nodal line Ω, the effective temperature T_eff, the surface gravitational acceleration log g, the projected rotational velocity vsini, the mass m, the radius R, the angular diameter θ, the bolometric magnitude M_BOL, the Johnson V magnitude and colour indices V, B−V, U−B, the dereddened Johnson V magnitude and colour index V₀, B₀−V₀, and the parallax π. Sources: RV solution of the RV curve presented in Table 5, SP comparison of the observed and synthetic spectra presented in Table 7, LC solution of the light curve presented in Table 9, IF solution of the V² and T₃φ presented in Table 11, HP. the Hipparcos parallax π = 15.60 ± 1.04 mas. The parallaxes: π_a1 estimated from the size of the semi-major axis of orbit 1 (physical and angular), π_a2 estimated from the size of the semi-major axis of orbit 2 (physical and angular), π_DM,Aa estimated from the distance modulus of component Aa, π_DM,Ab estimated from the distance modulus of component Ab, π_DM,Ab estimated from the distance modulus of component B.