Fig. 11.

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Spatial distribution for the MS star (purple) and the BD (green) material at the end of the AM (left column) and BM (right column) merger scenarios. Particles in blue have radial velocity larger than the local escape velocity and all of them belong to the MS star. Every row shows a thin slice in a different plane of the same 3D distribution. All panels have a size of 2 × 1012 cm per side and the black circle in the center of each panel shows the original radius of the MS star.
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