Fig. 3
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Orbits, eccentricities and inclinations of disk particles before and after stellar impacts. First column shows the initial conditions for all experiments. Frames in Cols. 2–5 correspond to resulting orbital parameters under the effect of a single 0.4 M⊙ and four 0.1 M⊙ encounters on a planetary disk with a radius of 100 a.u. The number of disk particles is equal to 4000.
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