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Fig. 1


Spatial distribution (in an arbitrary projection) of the dark matter (upper panels), gas (middle panels) and stars (lower panels) in our simulation, in a cube of 2.5 cMpc on a side and for redshifts z = 2,1,0.5 and 0. The R200 of G1 (solid line) and G2 (dashed line) at each redshift are indicated, and the colour scale (of each mass component) is fixed in order to highlight differences in the distributions at different times. The plots correspond to run CS, but results at these scales are very similar for both simulations.

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