Total flux maps (first row from the top) at three different wavelengths, the VIS (left column), NIR (central column), and submm (right column) range, for the reference model based on the temperature distribution T_MC. The total flux maps were calculated as the sum of three individual flux maps corresponding to the contributions of the star (second row), self-scattered thermal dust emission (third row), and direct unscattered thermal dust emission (fourth row). Respective labels of the individual maps and their interrelationship are indicated at the right of each row. The total flux of each model, given in Jansky, is indicated in the upper-right corner of each total flux map. Percentage values in the upper-right corner of the flux maps below (rows 2, 3, and 4), denote the contribution of the respective radiation source to the total flux of the model.