Dependence of the interferometric quantities (visibilities, wavelength-differencial phases, and closure phases) of our best-fit disk-wind model 5 (see Table A.1) on the inclination angle i: 10, 15, and 20° from left to right for the PA 300° of the disk (see Fig. 7). In contrast to Fig. 7, the Brγ line profiles are given without convolution with the instrumental profile of the AMBER spectrograph for clearer visibility of the theoretical line profiles.