Fig. 10
Azimuthal velocity profiles at R = 5.4 and 10.8 kpc in the simulation of the MW-like galaxy of Kawata et al. (2014b). Filled symbols are the tangential velocity of the gas component of the simulated galaxy. The green solid line is the nonuniform circular velocity predicted from the asymmetric methodology, the violet dashed line is the uniform circular motion.
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