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Fig. 6.


Mass accretion history of stars (dashed lines), and gas (dotted lines) enclosed within r <  R200, z, normalised by the baryonic mass at z = 0 as a function of redshift for the five haloes (Aq-A-SPH red, Aq-C-SPH brown, Aq-D-SPH green, Aq-E-SPH blue and Aq-C-M14 grey). We also plot the contribution of both together (i.e. baryons, filled lines). The grey horizontal line is shown to give a reference of the redshift at which each halo reach the 80% of the present baryonic mass.

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