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Simulations, Data Analysis and Algorithms

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Table 1 Simulation initial conditions and main results

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

\(\boldsymbol{M}_{\boldsymbol{1}}\) ( \(\boldsymbol{M_{\odot }}\) ) \(\boldsymbol{M}_{\boldsymbol{\mathrm{ej}}}\) ( \(\boldsymbol{M_{\odot }}\) ) a ( \(\boldsymbol{R_{\odot }}\) ) \(\boldsymbol{\Delta M}_{\boldsymbol{2}}\) ( \(\boldsymbol{M_{\odot }}\) ) \(\boldsymbol{v}_{\boldsymbol{\mathrm{im}}}\) (km s −1 )
4.0 2.6 4.5 0.021 78
4.0 2.6 5.5 0.013 57
4.0 2.6 6.5 0.0096 47
3.0 1.6 4.0 0.037 83
3.0 1.6 5.0 0.020 60
3.0 1.6 6.0 0.013 48
  1. The first three columns indicate the initial conditions, where \(M_{1}\) is the mass of the primary (helium star) and before the supernova, \(M_{\mathrm{ej}}\) is the total ejecta mass, and a is the initial orbital separation. The last two columns are the amount of mass stripped from the companion star and the (magnitude of the) impact velocity.