Notes. The parameters are obtained by solving the inverse problem for the Roche model with an accretion disk around the more massive (hotter) gainer in the critical non-synchronous rotation regime (Djurašević 1992a,b, 1996). Fixed Parameters: q = ℳ_c/ℳ_h = 0.22 – mass ratio of the components, T_c = 4400 K – temperature of the less massive (cooler) donor, F_c = 1.0 – filling factor for the critical Roche lobe of the donor, f_c = 1.00 – non-synchronous rotation coefficients of the donor, F_h = R_h/R_zc – filling factor for the critical non-synchronous lobe of the hotter, more massive gainer (ratio of the stellar polar radius to the critical Roche lobe radius along z-axis for a star in critical non-synchronous rotation regime), β_h = 0.25, β_c = 0.08 – gravity-darkening coefficients of the components, A_h = 1.0, A_c = 0.5 – albedo coefficients of the components. Note: n – number of observations, Σ(O − C)² – final sum of squares of residuals between observed (LCO) and synthetic (LCC) light curves, σ_rms – root mean square of the residuals, i – orbit inclination (in arc degrees), F_d = R_d/R_yc – disk dimension factor (the ratio of the disk radius to the critical Roche lobe radius along y-axis), T_d – disk-edge temperature, d_e, d_c, – disk thicknesses (at the edge and at the center of the disk, respectively) in the units of the distance between the components, a_T – disk temperature distribution coefficient, f_h – non-synchronous rotation coefficient of the more massive gainer (in the critical non-synchronous rotation regime), T_h – temperature of the gainer, A_hs, bs = T_hs, bs/T_d – hot spot temperature coefficients, θ_hs, bs and λ_hs, bs – spot angular dimension and longitude (in arc degrees), θ_rad – angle between the line perpendicular to the local disk edge surface and the direction of the hot spot maximum radiation, Ω_h, c – dimensionless surface potentials of the hotter gainer and cooler donor, ℳ_h,c[ℳ_⊙], ℛ_h,c [R_⊙] – stellar masses and mean radii of stars in solar units, log g_h, c – logarithm (base 10) of the system components effective gravity, – absolute stellar bolometric magnitudes, a_orb [R_⊙], ℛ_d [R_⊙], d_e[R_⊙], d_c[R_⊙] – orbital semi-major axis, disk radius, and disk thicknesses at its edge and center, respectively, given in solar units.