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Investigating the Globally Collapsing Hub–Filament Cloud G326.611+0.811

  • Authors: Yu-Xin He, Hong-Li Liu, Xin-Di Tang, Sheng-Li Qin, Jian-Jun Zhou, Jarken Esimbek, Si-Rong Pan, Da-Lei Li, Meng-Ke Zhao, Wei-Guang Ji, Toktarkhan Komesh

Yu-Xin He et al 2023 The Astrophysical Journal 957 .

  • Provider: AAS Journals

Caption: Figure 2.

(a) Averaged spectra of 13CO (J = 2–1) (black) and C18O (J = 2–1) (red) over the hub–filament cloud of G326. The intensity of C18O (J = 2–1) has been reduced by a scale factor of 5 for ease of viewing. The vertical dashed lines show the velocity interval −41.5 to −33.0 km s−1 over which the infrared dark hub–filament cloud of G326 extends. (b) Beam-averaged spectra of 13CO (J = 2–1) (black) and C18O (J = 2–1) (red) for C1. (c) Same as panel (b), but for C2. (d) Same as panel (b), but for C3.

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