Radio observations show gas in Mon R2 flows from inter-filament regions into filaments and the central hub, with along-filament accretion rates 6.8 times cross-filament rates in filaments and 1.5 times in inter-filament gas.
A., Andr 'e, P., et al.2014
4 Pith papers cite this work, alongside 211 external citations. Polarity classification is still indexing.
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Multi-wavelength observations identify a compact hub-filament system in G286.21+0.17 whose core properties follow steep radial power laws consistent with competitive accretion.
Young star clusters in the NGC 628 simulation inherit a filament mass power-law index of -1.35 at formation via gravitational fragmentation and evolve to -1.55 after 60 Myr.
Synthetic Herschel observations from simulations yield 8832 filaments hosting 94% of clumps, with power-law mass and length distributions and a density relation qualitatively matching the Hi-GAL survey.
citing papers explorer
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From inter-filamentary gas to filaments and hubs: gas flows in the Mon R2 hub-filament system
Radio observations show gas in Mon R2 flows from inter-filament regions into filaments and the central hub, with along-filament accretion rates 6.8 times cross-filament rates in filaments and 1.5 times in inter-filament gas.
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Discovery of a Compact Hub-Filament System in G286.21+0.17 with JWST and ALMA: Insights into Protocluster Formation and Competitive Accretion
Multi-wavelength observations identify a compact hub-filament system in G286.21+0.17 whose core properties follow steep radial power laws consistent with competitive accretion.
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Revealing the Connection Between the Filamentary Hierarchy and Star Cluster Formation in a Simulated NGC 628 Galaxy
Young star clusters in the NGC 628 simulation inherit a filament mass power-law index of -1.35 at formation via gravitational fragmentation and evolve to -1.55 after 60 Myr.
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From filaments to clumps: filament properties with synthetic Herschel observations
Synthetic Herschel observations from simulations yield 8832 filaments hosting 94% of clumps, with power-law mass and length distributions and a density relation qualitatively matching the Hi-GAL survey.