(General comments about the panels as in Fig. A.1.) ESO 297-G012: this is the southern galaxy of the system IRAS F01341-3735. The Hα emission is oriented perpendicular to the major stellar axis as traced by the continuum image. Although a rotation component is visible in the velocity field along the major photometrical axis, its structure, as well as that of the velocity dispersion map, is irregular. In an inner region (~1 kpc²), the spectra have been fitted with two components, with the broad component blueshifted by ~50 km s^-1. The scale is 0.352 kpc/′′.