Figure 11
From: Simulations of stripped core-collapse supernovae in close binaries
A 3D rendering of the gas density in the system \(\pmb{10^{3} \text{ s}}\) after the supernova, viewed down the x -axis (a; the original axis of the binary) and y -axis (b). The companion is still distorted due to the impact, and has produced a hole in the expanding ejecta. We used the software Mayavi2 (Ramachandran and Varoquaux 2011) for the visualisation.