Fig. 6.
Top two images: synthetic infrared emission maps of the bow shock on a logarithmic colour scale (in units of MJy ster−1), generated from the 1b simulation for viewing angle angles of 45° and 60°. Both synthetic images are generated after 0.2135 Myr of evolution and smoothed to the angular resolution of Spitzer of 6 arcsec. The coordinates are in parsecs relative to the position of the star. The black cross shows the position of the ionizing star. Bottom plot: Spitzer 24 μm image of the Bubble Nebula.
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