Fig. 7

Location and widths of the strongest resonances in the planetary regime weakly perturbed by the galactic tides. The semi-major axis taken as parameter is a = 500 au. For better visibility, the perihelion distance of the resonance centre is directly used as horizontal axis. Top: location and width in inclination (filled areas). Bottom: upper and lower half widths in perihelion distance, for a centre given by the horizontal axis.
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