Image Details

Choose export citation format:

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 6.

Correlation matrix of different observational (left) and derived physical (right) parameters of MCs. The observational parameters corresponding to indices 0 through 30 are (0) log Vspan; (1) R2, (2) θ, (3) e, and (4) log ﹩{l}_{{\rm{\max }},{\rm{ang}}}﹩ for 12CO; (5) R2, (6) θ, (7) e, and (8) log lmaj,ang for 13CO; (9) R2, (10) θ, (11) e, and (12) log lmaj,ang for C18O; (13–15) log σv(12CO, 13CO, C18O); (16–18) log ﹩\overline{W}﹩(12CO, 13CO, C18O); (19–21) log Tpeak(12CO, 13CO, C18O); (22–24) log Wpeak(12CO, 13CO, C18O); (25–27) log ﹩{\overline{T}}_{{\rm{peak}}}﹩(12CO, 13CO, C18O); and (28–30) log A(12CO, 13CO, C18O). The physical parameters corresponding to indices 0 through 36 are (0) R2, (1) θ, (2) e, and (3) log lmaj for 12CO; (4) R2, (5) θ, (6) e, and (7) log lmaj for 13CO; (8) R2, (9) θ, (10) e, and (11) log lmaj for C18O; (12–14) log σv(12CO, 13CO, C18O); (15) D; (16) Rgal; (17) log zgal; (18) log Tex; (19–21) log τ(12CO, 13CO, C18O); (22–24) log ﹩N{({{\rm{H}}}_{2})}_{(12,13,18)}﹩; (25–27) log M12,13,18; (28) log αvir,12; (29) log αvir,13; (30) log αvir,18; (31–33) log Mach(12CO, 13CO, C18O); (34–35) log f(13CO, C18O); and (36) log XCO.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse