Fig. 7
The WR-LBV interaction in low resolution. This figure shows the density in cgs. as well as the velocity field for simulation B1 after 4010 and 11 800 years. In the left panel, the shell mainly shows small Vishniac instabilities. In the right panel, some evidence of RT instabilities is visible, but unlike for the WR-RSG interaction (Figs. 3 and 4), they are small compared to the size of the shell.
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