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Fig. 4

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Left panels: morpho-kinematic PA misalignments at different regions of the galaxy against the stellar mass for both the stellar (top panel) and the ionised gas (bottom panel) components in a subsample of low-inclined galaxies. In each of these panels, the red points represent the morpho-kinematic PA misalignment between PA (see Table B.1) and PAkin up to rin. Blue points represent the morpho-kinematic misalignment between PA and PAkin up to rout (see Sect. 4.3 for details). Filled circles, squares, and stars represent unbarred, weakly barred and strongly barred galaxies, respectively. Right panels: difference between the kinematic PA derived at rin and rout against the stellar mass for both the stellar (top panel) and the ionised gas (bottom panel) components. In the panels we highlight those objects with larger misalignments.

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