Fig. 7
l−v diagrams at b = 0° for the J = 1−0 CO emission line in the regions QI (top row) and QIV (bottom row) of the Milky Way. The panels on the left show our model, the panels on the right show the CO data of Dame et al. (2001). Both datasets are smoothed to the angular resolution of 1° × 1° and the velocity resolution of 2 km s-1. Brightness temperature contours range from 0.03 K (or 3 times the rms noise) to 15.36 K in multiples of 2.
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