Dependence of the depths of eclipses in EE Cep system on precession. Photometry obtained during epochs 0–10 is shown as circular symbols. The solid and dashed lines delineate two models of the changes in eclipse depth as a function of orbital phase, generated using our numerical code. In these two cases, the precession periods P_prec are 10.8 P_orb and 11.8 P_orb, respectively. At the bottom, the spatial configurations of the disk and the star in four special cases, denoted by the letters a, b, c, and d, are shown.