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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 4.

The same as Figure 3, but for derived physical parameters. We select eight derived physical parameters to show as examples. These parameters are ﹩{l}_{{\rm{maj}}}{{\rm{(}}}^{13}{\rm{CO)}}﹩, ﹩{{\rm{N(H}}}_{2}{{\rm{)}}}_{12}﹩, M13, M18, ﹩{\alpha }_{{\rm{vir,}}{{\rm{12}}}}﹩, ﹩{\alpha }_{{{\rm{vir, 13}}}}﹩, Mach(C18O), and XCO. All parameter distributions and the corresponding fitted parameters are available in Science Data Bank at doi:10.57760/sciencedb.32354.

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