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Fig. 9


Difference between the morphological and kinematic position angles as a function of the disk inclination for the sample of spatially resolved galaxies in the MUSE-HDFS. Dots are color-coded as a function of the relative size of the disk (effective radius derived from Galfit) with respect to the FWHM of the MUSE PSF. Labels indicate the galaxy ID. The dashed line indicate the mean value of the sample.

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