Fig. 10
Detailed comparison of three fields in the strip perpendicular to the Galactic plane between lII = 195° and lII = 205°, as shown in Fig. 2. The three areas include: the Galactic plane, the Orion SFRs, and the Gould Belt, respectively. Histograms are cumulative, not stacked, i.e., each histogram includes the stars in all subcategory histograms.
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