Snapshot from the Z01 simulation used to generate synthetic images of ζ Ophiuchi at angles from 0° – 90° with respect to the direction of stellar motion. The first row shows the 24μm emission, the second row shows the 70μm emission, the third row shows the Hα emission, the fourth row shows the emission measure, the fifth row shows the 6Ghz Radio, and the sixth row shows the soft X-ray emission. From left to right, the projection angles are 0°, 15°, 30°, 45°, 60°, 75°, and 90° with respect to the x-axis. Each image is centred on the star (white cross) and is roughly 1.0×1.0 parsec.