Three-dimensional simulations of clump formation in stellar wind collisions

Keyphrases

• Stellar Winds 100%
• Three Dimensional Simulation 100%
• Wind Speed 66%
• Thin Shell 66%
• Formation Process 66%
• Shell Instability 66%
• Order of Magnitude 33%
• Three-order 33%
• High-resolution 33%
• Three-dimensional (3D) 33%
• Ejection 33%
• Hydrodynamic Instability 33%
• Galaxies 33%
• Galactic Center 33%
• Hydrodynamic Simulation 33%
• Grid-based 33%
• RAMSES 33%
• Formation Properties 33%
• Degree of Asymmetry 33%
• Speed Distribution 33%
• Dense Materials 33%
• Adaptive Mesh Refinement 33%
• Adiabatic Regime 33%
• Radiative Regime 33%
• Thermodynamic State 33%
• Supermassive Black Hole (SMBH) 33%

INIS

• wind 100%
• simulation 100%
• collisions 100%
• stellar winds 100%
• speed 75%
• instability 75%
• shells 50%
• nonlinear problems 50%
• dispersions 25%
• distribution 25%
• increasing 25%
• thermodynamics 25%
• resolution 25%
• asymmetry 25%
• grids 25%
• plasma 25%
• black holes 25%
• hydrodynamics 25%
• galaxies 25%

Physics

• Stellar Wind 100%
• Wind Velocity 66%
• Theoretical Model 33%
• Parsec 33%
• Supermassive Black Holes 33%
• Galactic Center 33%
• High Resolution 33%
• Hydrodynamical Simulations 33%
• Hydrodynamics 33%
• Thermodynamics 33%