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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 11.

Galactic-latitude dependence of source-averaged gas–dust quantities and velocity-component statistics. Panels (a)–(f) show the binned median trends of (a) ﹩{N}_{{}^{13}{\rm{CO}}}﹩, (b) ﹩{N}_{{{\rm{H}}}_{2}-{\rm{dust}}}﹩, (c) ﹩{I}_{{}^{12}{\rm{CO}}}﹩, (d) the catalog dust temperature together with the 13CO-intensity-weighted excitation temperature, (e) XCO, and (f) [H2]/[13CO]. Error bars indicate the corresponding median absolute deviations. In panels (b), (e), and (f), gray symbols use the 95% upper confidence limit of ﹩{N}_{{{\rm{H}}}_{2}-{\rm{dust}}}﹩, while blue symbols show the nominal catalog estimate multiplied by constant factors for display only, as indicated in the legends. Panel (g) presents the Galactic-latitude distributions of PGCCs, 13CO velocity components, and 12CO velocity components, together with the mean numbers of 12CO components per PGCC and 13CO components per 13CO-detected PGCC. Numbers above the bars denote the counts of PGCCs with multiple 12CO velocity components in each latitude bin.

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