Fig. 11

Model velocity map for a geometrically thin disk undergoing both Keplerian rotation and expansion with radial velocity proportional to the radius. Fiducial values have been assumed for the parameters (see text). The map has been rotated by 45° to ease the comparison with Fig. 10. The dotted and dashed lines indicate the directions of the two velocity gradients defined by the blue- and redshifted velocity peaks.
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