The interaction of core-collapse supernova ejecta with a companion star

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Fig. 9

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As Figs. 7 and 8, but as a function of the SN ejecta mass. All parameters (binary separation of 5.48 R_⊙ and a SN explosion energy of 1.0 × 10⁵¹ erg) except the SN ejecta mass (M_ej) are kept constant. Different values of M_ej = 0.7, 1.4, 2.5, 4.0, and 5.0 M_⊙ are applied.

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