Fig. 3
Amount of mass removed from the companion star (top panel) and the impact velocity caused by the SN ejecta (bottom panel) as a function of time after the SN explosion in our impact simulations of a G/K-dwarf companion (M2 = 0.9 M⊙) with an initial binary separation of a = 5.48 R⊙ ≈ 7.1R2 ≈ 2.0amin. Here, amin is the minimum possible separation of the binary system.
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