Fig. 6.
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Position-velocity maps for the CO(2-1) of each object for 1″-width pseudo-slits along three different positions: kinematics major and minor axis (first two columns) and along the double-peak (dp) region (last column). We added the individual LoS velocities obtained for the Gaussian components c1 (blue circles) and c2 (orange circles) fit to the spectral profiles. The bluish-green lines correspond to the global rotating disk model fit to the single-peak (sp) region (first three rows in Table 2). For NGC 6860, three models are shown, which were fit using data from the ring (bluish-green line), from the bar (dot-dashed black line), and combining data from both ring and bar (long dashed black line). For MCG -01-24-012, we also added curves from two models fit in the double-peak region, one letting the PA free (short dashed black line) and the other with PA = 0° (dotted black line).
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