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The TOP-SCOPE Survey of Planck Galactic Cold Clumps: Molecular Gas Properties

  • Authors: Yang Yuebin, Jarken Esimbek, Tie Liu, Willem Baan, Xunchuan Liu, Kee-Tae Kim, Gang Wu, Xindi Tang, Jianjun Zhou, Dalei Li, Yuxin He, Sung-Ju Kang, Yingxiu Ma, Dongdong Zhou

Yang Yuebin et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 14.

The source-averaged 13CO-intensity-weighted Mach number, ﹩{\langle { \mathcal M }\rangle }_{{}^{13}{\rm{CO}}}﹩, vs. the dust-derived H2 column density, ﹩{N}_{{{\rm{H}}}_{2}-{\rm{dust}}}﹩ (a), and the catalog dust temperature, Tdust (b). Panel (c) shows Tdust vs. ﹩{N}_{{{\rm{H}}}_{2}-{\rm{dust}}}﹩ for the same sample. Black points represent individual PGCCs, red symbols indicate median values in logarithmic bins, and error bars show the corresponding median absolute deviations. Gray and blue contours trace the kernel-density distribution.

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