Fig. 5
The WISE 12-μm image over a field of 18′ × 33′ encompassing the cloud in which IRAS 07422 is located. The contours in black, white and grey show the boundaries where the emission from the cloud falls to 15%, 40% and 85% respectively of the peak flux in the bar. Most of the star formation happening within this cloud is in the region within the white contours.
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