Comparison of various radial profiles for the stellar component of five models with different AGN feedback parameters: mdf018 (no AGN), mdf789 (T_AGN = 5 × 10⁶ K, ρ_AGN = 1 M_⊙/pc³), mdf732 (T_AGN = 1 × 10⁷ K, ρ_AGN = 1 M_⊙/pc³), mdf788 (T_AGN = 2 × 10⁷ K, ρ_AGN = 1 M_⊙/pc³), and mdf791 (T_AGN = 1 × 10⁷ K, ρ_AGN = 2 M_⊙/pc³), all at t = 10 Gyr. From left to right and top to bottom: surface density, median of the absolute value of z, which is a good approximation for thickness (Sotnikova & Rodionov 2006), mean value of the azimuthal velocity and radial velocity dispersion. The inlay in the upper left panel shows the surface density in the innermost region (within 3 kpc).