Fig. 11.

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H2 S(5) p–v diagrams extracted along the kinematic major (top) and minor axes (bottom). The gray scale and blue contours are the observations, and red contours represent the fit 3DBAROLO rotating disk model. Yellow dots show the fit rotation curve. In the central ±0.5″, some of the blueshifted velocity structure might be due to residuals left from subtracting the AGN strong continuum. PAmaj is measured from north, counterclockwise, and on the receding half of the galaxy disk.
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