Fig. 14.
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Histogram of the probability density of the angle θ between the DM and baryonic angular momentum vectors for halos without clumps (blue bars) and halos hosting clumps (red bars) for the three last snapshots (corresponding to redshifts 19.5, 18.8 and 18). Error bars correspond to the Poissonian error. The fraction on the right-axis corresponds to the ratio of the number of halos hosting a clump versus the total number of halos.
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