Visualization of disk destruction: same as Fig. 7, but for later times of the disk evolution. Dotted, dashed, and solid lines corresponds to t = 90, 115, and 125 kyr of evolution, respectively. The upper panel corresponds to a simulation without radiative forces, while the lower panel includes them. Outflows and photoionization is accounted for in both simulations shown, both panels present the data from the large-scale mass reservoir simulations.