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Statistical Properties of Molecular Clouds in the Milky Way: Insights from Three-isotopologue CO Observations of the MWISP Project

  • Authors: Xin Zhou, Ji Yang, Qing-Zeng Yan, Yan Sun, Lixia Yuan, Yang Su, Xuepeng Chen, Shaobo Zhang

Xin Zhou et al 2026 The Astrophysical Journal Supplement Series 285 .

  • Provider: AAS Journals

Caption: Figure 9.

Same as Figure 8, but for derived physical parameters. The physical eigenparameters are ﹩\mathrm{log}\,{l}_{{\rm{maj}}}﹩(13CO), ﹩\mathrm{log}\,﹩N(H2)12, ﹩\mathrm{log}\,{M}_{18}﹩, ﹩\mathrm{log}\,{\alpha }_{{\rm{vir}}\,{\rm{12}}}﹩, ﹩\mathrm{log}\,{\alpha }_{{\rm{vir}}\,{\rm{13}}}﹩, and ﹩\mathrm{log}\,Mach﹩(C18O). The physical parameters are in log form, except for the morphological parameters (R2 and θ), distance D, Galactocentric distance Rgal, and height from the Galactic plane zgal. All fitted parameters are available in Science Data Bank at doi:10.57760/sciencedb.32354.

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