Notes. m denotes the mass; P_rot, the rotation period; i, the inclination of the stellar rotation axis with respect to the sky; Ω, the longitude of the ascending node of the star (i.e. equator); d, the distance; T_eff, the effective temperature; log g, the logarithm of surface gravity; β, bolometric gravity brightening exponent; γ, the systemic velocity; γ_LSR, the systemic velocity with respect to the local standard of rest; R_equiv, the equivalent radius; R_pole, the pole radius; R_equ, the equatorial radius; θ_equiv, the equivalent angular diameter; θ_pole, the polar angular diameter; θ_equ, the equatorial angular diameter; L, the luminosity; v_rot sin i, the projected rotation velocity; v_rot, the rotation velocity; and f, the rotation frequency.