Fig. 5.
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DiskFit results for NGC 4845. Top panels: pure rotation DiskFit model (flat disk). Middle panels: rotation plus radial motion DiskFit model. Bottom panels: bisymmetric DiskFit model. For every panel, the top left figure reports the data the top right represents the model, the bottom left the residual obtained subtracting the model from the data, and bottom low right figure the dispersion.
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