Evolution of galaxies in simulated cluster. Columns: results for different galaxies, with ID = 53, 80 and 81. Upper row: evolution of the dark, stellar and gas mass shown with the blue, red, and green lines, respectively. The data are the same as in Fig. 1, but the mass scale was adjusted to the range of stellar and gas masses. Second row: orbit of the galaxy within the cluster in terms of its distance from the cluster center in physical units. Third row: evolution of three structural properties of the galaxies, the axis ratios b/a (blue line) and c/a (red), and the triaxiality parameter T (green). Fourth row: rotation measure in terms of the fractional mass of stars on circular orbits f (blue) and the bar strength A₂ (red). Fifth row: g − r color and metallicity Z (in solar units, divided by 3 to fit the same scale as the color).