Dynamical accretion flows - ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters

Open Access

Fig. 7.

Theoretical spreading of the observed flow rate due to unknown inclination of the filament for a tube-like cylindrical filament model with a universal flow rate of $\dot{M} = 10^{- 4}$ $\dot{M} = 10^{-4}$ M_⊙ yr⁻¹ (marked as a vertical thin line). The probability distribution is generated for 60 bins, with a uniform binning width in log space.

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