Fig. 5
Modeling of the VEGA observations on 2010 October 17 (left) and 2012 September 21 (right). Top: observed (black circles) and modeled spectra for all disk-wind models (M1: dashed line; M2: dotted line; M3: solid line). The dash-dotted red line indicates the contribution of the magnetosphere to the profile for M3. Middle: same for differential visibilities. Bottom: same for differential phases. The spectral bin is represented by the red line in the bottom corner of each panel.
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