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Fig. 11.

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Radial profiles of the ALMA CO(3−2) median intensity (top panel), gas velocity dispersion (middle panel), and radial velocity (bottom panel) fitted with the 3DBAROLO model in Sect. 4.2. As explained by García-Burillo et al. (2019), the vertical error bars in the integrated CO(3−2) emission reflect the deviations from symmetry in the gas distribution.

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