Fig. A.10
(General comments about the panels as in Fig. A.1.) ESO 255-IG007: this is the southern galaxy of the system IRAS F06259-4708. It has a regular velocity field and the velocity dispersion map. One single Gaussian component is adequate to fit the Hα-[NII] emission lines of this galaxy. The scale is 0.769 kpc/′′.
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