Fig. 9

Bulk kinematic properties of the mock GC systems generated in the halos around Aq-B through Aq-E. Each row corresponds to the same Aquarius galaxy. The first column shows the distribution of kinematic ratios for all GC systems, regardless of the viewing angle. The second column shows the difference in the position angle between the angular momentum of the GC systems projected on the plane of the sky and the rotation axis determined via our analysis as a function of A/σ0. The third column shows the angular difference between the orientation of the 3D angular momenta of the mock GC systems and the angular momentum of the entire stellar halo located beyond 30 kpc in projection.
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