Brγ intensity distribution maps of our best disc-wind model P5 (see values of parameters in Table 3, Col. 3) in logarithmic scale (arbitrary units). Each panel shows the intensity map for a different radial velocity, indicated by a white label in units of km s^-1. X and Y coordinates on each map are in R_∗. The system axis inclination angle with respect to the line of sight is assumed to be 20° (see Table 2). Continuum emission from the disc and central star, located at coordinates 0, 0, are not shown.