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From Interfilamentary Gas to Filaments and Hubs: Gas Flows in the Monoceros R2 Hub–Filament System

  • Authors: Jihye Hwang, Doris Arzoumanian, Yoshito Shimajiri, Masahiro N. Machida, Shu-ichiro Inutsuka, M. S. N. Kumar, Shingo Nozaki, Kazuki Tokuda

Jihye Hwang et al 2026 The Astrophysical Journal Letters 1004 .

  • Provider: AAS Journals

Caption: Figure 8.

Top left: Fs and IFs overlaid on the H2 column density map obtained from Herschel data (the same as in Figure 1). The white dashed lines indicate the boundaries of the subregions we analyze in steps of 0.2 pc. Top right, bottom right, and bottom left: centroid velocities as a function of position along the arc, from west (0 pc) to north (2.5 pc), within the region between two radial distances from the hub center. The two radial distances are given in the upper left corners of each panel. The green vertical line indicates the position of the prestellar core located in F1.

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