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Fig. 6
Pixel-to-pixel comparison of NIR extinction and 13CO integrated line emission for the 38.94-00.46 (Dfg = 2.7 kpc) and 32.09+00.09 (Dfg = 8.0 kpc) complexes. The dotted line shows a typical ratio of these quantities for local molecular clouds (Pineda et al. 2008).
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