Fig. 6

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Velocity-integrated intensity maps of the 13CO (J =2−1) emission. Bottom panel: Velocity-integrated intensity map of G323.18a (blue contours integrated from −69.0 to −65.5 km s−1 starting at 2 K km s−1 with an increment of 5.5 K km s−1), G323.18b (white contours, integrated from −65.5 to 64.0kms−1 starting a 2 K km s−1 with an increment of 3.8 Kkm s−1), and G323.18c (red contours, integrated from −64 to −62 km s−1 starting at 2 K km s−1 with an increment of 2.3 K kms−1). The black circle denotes HII region G323.187+00.129 identified by Anderson et al. (2014). The yellow and red diamonds are prestellar and protostellar clumps from the Herschel Hi-Gal clump catalog, and the white crosses are ATLASGAL 870 µm clumps. The background is a three-color map with red, green, and blue for 24, 8, and 4.5 µm, respectively. Top panel: white contours start from 2 × 1021 cm−2 and increase in steps of 1.9 × 1021 cm−2. They display the distribution of the H2 column density of the dotted rectangle in the bottom panel. The background is the same as in the bottom panel.
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