Fig. 3
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Comparison between the number density fields in the supernova remnant models of a runaway 20 M⊙ (left-hand side) and a 35 M⊙ (right-hand side) star rotating with Ω⋆/ΩK = 0.1, moving with a velocity of v⋆ = 20 km s−1 (left column) and v⋆ = 40 km s−1 (right column). The green contour mark the parts of the SNRs, with a 50% contribution from the ejecta.
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