Fig. 3

h–k space evolution of parent belt particles (orange; abelt = 100 au; β = 0.0; e ≈ 0.0), and particlescreated in collisions of parent belt objects; with fragment β values of β = 0.01;0.03;0.05 (black), and 0.3 (blue). The belt is around a star of M = 1.92 M⊙, and the collisional fragments are perturbed by a mp = 2.5 MJup mass planet, with a = 20 au and e = 0.6 (left); a = 60 au and e = 0.2 (right). The initial distribution of particles created in the collisions (dashed line), and the position after a time T (solid line) are shown. In between steps are marked with faint colours.
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