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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 7.

Distribution of the beam detection fractions for the 12CO and 13CO (J = 1–0) lines (upper panel), and of the detection-fraction difference Δf = f12 − f13 (bottom panel). For each PGCC, ﹩{f}_{{\rm{\det }}}={N}_{{\rm{\det }}}/{N}_{{\rm{beam}}}﹩, where Nbeam is the total number of sampled beam positions associated with the source and ﹩{N}_{{\rm{\det }}}﹩ is the number of beam positions with detected line emission.

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