Fig. 15.

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Comparison of velocity profiles identified using the six different methods of dynamical decomposition as a function of cylindrical radius R of the IllustrisTNG galaxy disk. Top panel: Comparison of rotational velocity vϕ. The differences are more evident in the internal part of the disk. Middle panel: Comparison of the radial velocity profile vR. Bottom panel: Comparison of the vertical velocity profile vz. These two profiles adopt values around zero regardless of the method used.
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