Model images of the disk wind (model A2, top) and model images of the X-wind (Table 2, bottom) in the Brγ line at the radial velocity 0 km s^-1. The mass-loss rate used in both models is 10^-7  M_⊙ yr^-1. Edge-on (left) and pole-on (right) orientations are presented. The brightness scale is arbitrary and given in logarithmic units.