Notes. We show the moments of time for the systems shown in Fig. 3. The moments of time: the RGB accretion peak, t_RGB ; the AGB accretion peak, t_AGB ; the donor envelope loss, which causes the termination of wind, t_env ; the first formation of the sufficiently large disk, t_frm ; formation of the most massive disk, t_AGB, which is practically equal to t_AGB ; a depleted disk after the termination of wind, t_dpl, which is in between t_AGB and t_dec, where t_dec corresponds to the disk decay. We note that the values of t_RGB, t_AGB, and t_env are universal for all systems with a given donor, while the values t_frm, t_dpl, and t_dec are unique for the particular binary initial separation. Additionally, a disk in the system with donor M₁ = 1.7 M_⊙ is smaller than ~2 AU or vanishes at all during the interval from t = 1852.593 Myr upto t = 1959.618 Myr.