Observations show gas in Mon R2 flows into the hub along filaments at higher rates than across them, with at least 30% of inter-filamentary mass potentially moving to filaments.
A., Duarte-Cabral, A., et al.2013
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Simulations of the Aquila Rift show uneven clumps accreting gas and merging along filaments to form a fractal cluster whose velocity anisotropies, rotation, and expansion record the assembly history even after gas removal.
citing papers explorer
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From inter-filamentary gas to filaments and hubs: gas flows in the Mon R2 hub-filament system
Observations show gas in Mon R2 flows into the hub along filaments at higher rates than across them, with at least 30% of inter-filamentary mass potentially moving to filaments.
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Simulating Star Formation and Star Cluster Assembly in the Aquila Rift Using Archival Observations
Simulations of the Aquila Rift show uneven clumps accreting gas and merging along filaments to form a fractal cluster whose velocity anisotropies, rotation, and expansion record the assembly history even after gas removal.