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Fig. 8.

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Upper panels show the evolution of the average misalignment angle θc between the stellar and dark matter minor axis as a function of their θJ alignment at z = 0, for red (left panel) and blue (right panel) BGGs within the mass range MTot < 1013 M. The grey dotted line on the upper panels indicates an average angle of 90°, corresponding to random orientation. The lower panels illustrate the distribution of θJ for red (left panel) and blue (right panel) BGGs within that same mass range.

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