Fig. B.1.
From left to right: CO(1-0) velocity field of IRAS F08572+3915, the best fit model from dysmalpy, and the residual map between the two. The observed motions in IRAS F08572+3915 are not purely rotational, as expected from a system that is undergoing a major interaction and host a powerful nuclear outflow. Nonetheless, the best fit velocity field from the dysmalpy code does a reasonable job reproducing the major kinematics features of IRAS F08572+3915.
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