Figure 9
From: Simulations of stripped core-collapse supernovae in close binaries
Magnitude of the impact velocity, \(\pmb{v_{\mathrm {im}}}\) , imparted to the companion star as a function of orbital separation a . Markers and line styles correspond to those used in Figure 7. Again, as for Figure 7, the comparison with Liu et al. (2015) is not fully equivalent due to the slightly different ejecta mass and companion parameters.