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Fig. 2.

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Density distributions of all material (panels a–c) and of the bound companion material (panels d–f). The panels shows a slice in the orbital plane for three different times each. Colours indicate density as per the colour bar (right). The 3D hydrodynamical simulation of the SN ejecta-companion interaction shown here does not include binary orbital motion or stellar spin. All panels use the same length scales.

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