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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 9.

Mass accretion rates (﹩\dot{M}﹩; left) and velocity gradients (Δv; right) along (∥) and across (⊥) the Fs and IFs, measured in 0.2 pc steps (within the arcs shown in Figure 8) from the hub center. The red open circles in the left and right panels indicate ﹩{\dot{M}}_{\parallel }﹩ and Δv, respectively. The blue dots in the left and right panels indicate ﹩{\dot{M}}_{\perp }﹩ and Δv, respectively. The error bars in the right panel are the fitting errors. In the last row, we overplot the values of F3 and IF3, as they are identified as a continuous structure radially extending away from the hub. The larger circles indicate values in IF3.

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