Gas and star kinematics. First row: maps for the first component, and second row: second component detected in MaNGA data. First and second columns: respective ionised gas and stellar velocity fields (in km s⁻¹). The dotted black lines refer to the computed position angles. Third and fourth columns: respective velocity dispersion fields (in km s⁻¹) for the gas and the stars. As in Fig. 2, the black crosses indicate the position of the extinction-corrected Hα flux peak for the represented component.