Total removed companion mass (left panel), resulting impact velocity of the companion star (middle panel) and the amount of accreted contamination from the SN ejecta (right panel), as a function of initial binary separations for a G/K-dwarf (square symbols, M₂ = 0.9 M_⊙ and R₂ ≈ 0.77 R_⊙) and a late-type B-star (filled circle symbols, M₂ = 3.5 M_⊙ and R₂ ≈ 2.18 R_⊙) companion model. The results of our example model (Sect. 3) are shown with red filled square symbols. Power-law fits are also presented in each panel.