Fig. 10.
Comparison between the best-fit model for the EPG of NGC 3198 (top panels) and two models that use the same parameters but different values for h and dvϕ/dz (bottom panels). Contours are the same as in Fig. 6. Arrows show the locations where the models are inferior to the best-fit one. We have focussed on pv-slices where the differences are more evident.
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