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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 8.

Fitting results of various observational parameters as a linear function of six selected observational eigenparameters. The observational eigenparameters are ﹩\mathrm{log}\,{V}_{{\rm{span}}}﹩, R2(13CO), ﹩\mathrm{log}\,{l}_{{\rm{maj}},{\rm{ang}}}﹩(13CO), ﹩\mathrm{log}\,{T}_{{\rm{peak}}}﹩(13CO), ﹩\mathrm{log}\,{T}_{{\rm{peak}}}﹩(C18O), and ﹩\mathrm{log}\,{\overline{T}}_{{\rm{peak}}}﹩(C18O). These parameters are in log form, so the fit is equivalent to a power-law fit to the original parameters, except for the morphological parameters (R2 and θ). The fitting is weighted by the significance of ﹩\overline{W}﹩(12CO), indicated by colors from blue to red. The magnitude of ﹩\overline{W}﹩(12CO) is shown in its plot in the third row. All fitted parameters are available in Science Data Bank at doi:10.57760/sciencedb.32354.

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