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Simulations, Data Analysis and Algorithms

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Figure 11 | Computational Astrophysics and Cosmology

Figure 11

From: Simulations of stripped core-collapse supernovae in close binaries

Figure 11

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.

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