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Fig. 11

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Fraction of stars in multiple systems over the velocity dispersion of stars in the z-direction at the end of the simulation (T = 300 Myr) for the main model. The points are colour-coded according to the angular distance in degrees of the cylinder from the SC with respect to the Galactic centre. Positive values of ϕSC indicate the stellar populations in the leading T1 and T2 tails, while ϕSC < 0 indicate the trailing tail ones.

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