D-CAF simulations show that ongoing gas collapse during star formation shortens stellar crossing times, rendering gas expulsion more adiabatic and thereby regulating the survival and expansion rates of young stellar systems.
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4 Pith papers cite this work. Polarity classification is still indexing.
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2026 4representative citing papers
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.
Simulations show stars at the edges of stellar streams are more likely to retain unperturbed planetary systems than stars near the stream center.
N-body simulations show sub-virial fractal star clusters produce more captured asteroids and rogue objects than virialised Plummer clusters, while neither efficiently forms an Oort Cloud.
citing papers explorer
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Dynamical Cluster Assembly Framework (D-CAF): The Link Between Star Cluster Formation and Expansion Rates
D-CAF simulations show that ongoing gas collapse during star formation shortens stellar crossing times, rendering gas expulsion more adiabatic and thereby regulating the survival and expansion rates of young stellar systems.
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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.
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Life is But a Stream: The Distribution of Planetary Systems Along Stellar Streams and their Properties
Simulations show stars at the edges of stellar streams are more likely to retain unperturbed planetary systems than stars near the stream center.