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 |