[Fe VII] λ6087 channel maps of the circumnuclear region of Mrk 1044. The channels correspond to the sum of three spectral elements (covering 3.75 Å), whose central velocity in the rest frame of the galaxy is shown at the top of the panels. Photocentres were determined for each channel and their position is plotted in the lower-right panel if the signal within a diameter equal to twice the FWHM exceeds S/N = 6. Channels under this threshold are marked as having ‘No signal’. The photocentres in the lower-right panel are colour-coded according to the velocity of their channel map. The cross indicates the centre of the galaxy. The axes labels are in arcseconds. The grey contours indicating the stellar emission and the purple circles indicating the FWHM of the PSF are as in Fig. 2.