Maps of the [O III] (top panels) and Hα (bottom panels) emission line flux distribution in the Teacup galaxy. The fluxes of the total modelled line profile (left panels; same reported in Fig. 1) and of the first, narrower (centre panels) and the outflow (second plus third), broader Gaussian components (right panels) making up the total profile are reported. The colour intensity scale is the same for all the three maps of each line, as reported in the colour bar to the right. The contours in upper-left panel mark the VLA radio emission at 5.12 GHz from Harrison et al. (2015), same as in Fig. 1, right panel.