Gallery of blueshifted CO globules and emission structures detected toward Orion’s Veil bubble. The reddish color is the ¹²CO (2–1) emission integrated over the appropriate emission velocity range of each globule (spectra shown in Fig. 5). The bluish color is the 8 μm emission (extended PAH emission) imaged with Spitzer/IRAC at 2″ resolution. Each panel indicates the LSR velocity centroid of the CO line-profiles and a white-lined circle with the 11″ (~4500 AU) beam size of the CO observations. The images of the smaller CO globules display ¹²CO (2–1) intensity contours (in red) starting with the 5σ rms level (except for the brighter globules #5 and #9). In order to exhibit the bright rims (FUV-illuminated edges) of the larger and brighter CO globules, their images do not display CO emission contours (except for globule #5, where the contours help to locate the head of a more elongated structure). Globule #1 matches the position of YSO #1728 (magenta star, Megeath et al. 2012). Figure A.1 shows the same gallery but displaying the velocity-resolved [C II] 158 μm emission in bluish.