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Imprints of feedback in young gasless clusters?
R.~J. Parker, James Dale
Centre for Astrophysics Research (CAR)
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Article
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peer-review
32
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Keyphrases
Substructure
100%
Star Formation
100%
Gasless
100%
Hydrodynamic Simulation
100%
N-body Simulations
100%
Photoionization
50%
Mass Radius
50%
Surface Density
50%
Structure Evolution
50%
Mass Loss
50%
Sinking Particles
50%
Star Clusters
50%
Virion
50%
Central Density
50%
Initial Velocity
50%
Relaxation Time
50%
Dynamical Evolution
50%
Physics
Hydrodynamical Simulations
100%
N-Body Simulations
100%
Star Formation
100%
Relaxation Time
50%
Photoionization
50%
Stellar Evolution
50%
Dynamical Evolution
50%
Star Cloud
50%