Time evolution of the (1) total cold gas mass (defined as T ≤ 10^4.5 K) in the simulation, (2) the cold gas in the tail, (3) the cold gas associated with the galactic disc, and (4) the total mass of stars formed since t = 2 Gyr. As expected from idealised simulations of cloud-wind interactions in the regime of large clouds, the cold gas mass of the tail increases after entering the cluster until a time close to the closest central passage. Continued star formation and enhanced ram-pressure stripping of the ISM during the central passage causes a drop of the cold gas in the disc and tail.