Morphology of the ICs made out of disrupted satellite stellar material resulting in models with mass ratio 1:6 (models a–f in Table 3). Surface density maps of the stars originally from the satellite in the final remnants are presented, using a face-on and an edge-on view (left and right columns in each model, respectively). A rainbow colour palette is used to represent different surface density levels on a logarithmic scale, with redder colours indicating higher values. The levels of the colour scale differ from panel to panel, as they have been set automatically to ensure an adequate sampling of the dynamical range of the surface density shown in each map. Spatial scales in both axes are provided in simulation units. The radial extent of each independent IC (i.e., characterized by an unique exponential profile, see Sect. 3.2.1) are marked with dashed lines in each map.