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Fig. 3.

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Final (t = 300tDyn) density profiles from MOND simulations (top panels) and the DM halo of the ENS (bottom panels) for cored γ0 = 0 (left), moderately cuspy γ = 1 (centre), and clumpy (right) initial conditions. The increasing initial values of the virial ratio in the models with spherical initial conditions with γ = 0 and 1 are mapped with increasingly lighter tones of blue and green, respectively. All clumpy initial conditions start with 2K0/|W|0 = 0.1.

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