(General comments about the panels as in Fig. A.1.) IRAS F06259-4708 (ESO 255-IG007): two VIMOS pointings were used during the observation of this triple system. The two brightest galaxies, the northern and the central ones, are separated by a distance of ~11 kpc, while the third one is located at ~13 kpc to the south from the central galaxy (see next panel). The present panels correspond to the northern and central galaxies, which show a regular velocity field pattern. The scale is of 0.769 kpc/′′.