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Fig. 2


Comparison of various radial profiles for the stellar component of five models with different AGN feedback parameters: mdf018 (no AGN), mdf789 (TAGN = 5 × 106 K, ρAGN = 1 M/pc3), mdf732 (TAGN = 1 × 107 K, ρAGN = 1 M/pc3), mdf788 (TAGN = 2 × 107 K, ρAGN = 1 M/pc3), and mdf791 (TAGN = 1 × 107 K, ρAGN = 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).

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