Fig. 14.
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Distributions of particle trajectories sampling the outflow from the central engine. The top panels show the axisymmetric and perturbed kilonova models, while bottom panels show the fiducial thin and thick models. In the 3D-Thin model, the cumulative ejected mass is quantitatively similar to that in the perturbed 3D-kn-p model. The same holds for 3D-Thick and 3D-kn models.
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