Fig. 5
3D simulation the WR-RSG interaction in low resolution (A3). From left to right: density in cgs of the CSM after 7920 and 39 200 years. This figure shows slices through the 3D grid. These results closely resemble Fig. 3, which has the same resolution in 2D. However, the instabilities in the 3D model are more pronounced than in 2D and develop quicker.
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