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CO Structures with Narrow Lines in Nearby Quiescent Regions

  • Authors: Ruilin Xia, Yang Su, Shiyu Zhang, Xuepeng Chen, Ji Yang, Yan Gong, Yuehui Ma, Yan Sun, Min Fang, Fujun Du, Shaobo Zhang, Xin Zhou, Lixia Yuan, Qing-Zeng Yan, Li Sun, Jiancheng Feng

Ruilin Xia et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 4.

Global distribution of the 57 structures. The top panel shows their positions in Galactic longitude–latitude (lb) space, while the bottom panel displays their distribution in longitude–velocity (lv). The symbols are the same as in Figure 1, with the color representing the observed 12CO line width. The light-gold shaded region in the lb panel marks spatial concentrations (l = 10°–50° and l = 100°–180°), while that in the lv panel corresponds to the velocity confinement (∣VLSR∣ ≤ 10 km s−1).

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