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Fig. 3


Histogram of R/Re for the resolved galaxies of our sample, where R is the maximum radius where we get a measurement of the velocity and Re is the effective radius. Only galaxies for which it is possible to fit a light profile with GALFITare shown. The galaxies that do not show a velocity gradient are in orange and the galaxies for which it is possible to fit a kinematic model (velocity gradient) are presented in blue.

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