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Fig. B.2


Similar to Figs. 3 and 6 but for simulation C with an external magnetic field of 10 μG. Because the supernova expansion is spherical and the outer boundary of the bubble is strongly ellipsoid, the supernova will first collide with the outer shell at the “waist” of the bubble, noticeable on the left side of the right panel. In fact, on the right side of the right panel, the supernova is already moving back toward the centre in the perpendicular direction, whereas it is still expanding in the direction parallel to the field.

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