Fig. 5
3D volumetric rendering of the density in the numerical model of SN1987A Orlando et al. (2015), at 15 yr (around Day 5500) after the supernova explosion. The three panels show the rendering at three different angles (see upper left corner of each panel) between the line of sight and the axis of the H ii region surrounding SN1987A. The colour-scale is normalised to the maximum value in each panel.
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