Comparison of the orbital characteristics of Galactic globular clusters integrated in Model I versus Model II. From top-left to bottom-right: pericentres Rmin, apocentres Rmax, maximum vertical distance from the plane zmax, period of vertical oscillations, and 3D eccentricities are given. The insets in some of the plots show a zoom in the inner regions. In all the plots, the y-axis shows the difference between Model II and Model I, relative to Model I. Distances are in kpc, time in units of 108 yr.
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