Open Access

Fig. 4


Mean azimuthal velocity (top) and orbital eccentricity, e ≡ (rapo − rperi)/(rapo + rperi), (bottom) of the GCs as functions of distance from the clump orbital plane in the end state of the fiducial run, where rapo and rperi are apo- and peri-center distances, respectively. Each line indicates a radial range in cylindrical coordinate, R. In the bottom panel, GCs rotating prograde and retrograde are separately plotted; the thick and thin lines correspond to prograde and retrograde ones, respectively.

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