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A Study of the Physical Properties and Star Formation Activity of a Large Sample of Molecular Clouds. I. Distances

  • Authors: Juan Mei, Min Fang, Miaomiao Zhang, Qing-Zeng Yan, Lixia Yuan, Xuepeng Chen, Zhiwei Chen, Yang Su, Shiyu Zhang, Zhibo Jiang, Ji Yang

Juan Mei et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 6.

Distance of MWISP G211.613+02.405+007.49 based on the AV versus WCO Pearson correlation from distance-sliced dust map. Panels (a), (b), and (d) are identical to those in Figure 3 and are described in detail in its caption. (c) The variation of the correlation coefficient at different distance slices. The blue line represents the correlation variation calculated with a 20% distance interval, while the red line shows a finer 5% interval. The black solid line indicates the estimated distance and the black dashed lines depict the uncertainty of the cloud distance.

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