Fig. 5
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Thermal dust emission maps from the final snapshot of our simulation, showing surface brightness at 11 µm on a logarithmic scale. The colour bar shows log10 I11 µm/(MJy ster−1). The radiation sources heating the dust are the RSG at the origin (orange star) and two sources indicated by the blue stars at x = 0.32 pc and z = ±0.32 pc.
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