Two-dimensional distribution of the total (HI, H₂, HII, He, and metals; upper left panel), ionised (upper right), atomic (lower left), and molecular (lower right) gas components of the simulated galaxy undergoing a wind of 2000 km s⁻¹, 150 Myr after the beginning of the interaction. The model galaxy is orientated as IC 3476 on the plane of the sky. The cyan cross in the upper left panel shows the stellar centre, the contours the stellar disc, while those in the lower panels show the distribution of the star-forming regions. The green arrow indicates the direction of the wind.