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.
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