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Simulations, Data Analysis and Algorithms

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Figure 13 | Computational Astrophysics and Cosmology

Figure 13

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

Figure 13

Density (left-hand axis) and internal energy (right-hand axis) of the companion star before (dashed lines) and 7828 s after (solid lines) the supernova explosion. These properties were determined by averaging across radial shells concentric with the centre of mass of the companion. All SPH particles bound to the companion were within a radius of \(4.5 R_{\odot }\).

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