Evolution of supernovae-driven superbubbles with conduction and cooling

Engineering

• Energy Engineering 100%
• Evaporation Rate 100%
• Cooling Rate 100%
• Temporal Evolution 50%
• Hydrodynamics 50%
• Mass Transfer 50%
• Heat Flux 50%
• Conductive 50%
• Similarities 50%
• Hot Gas 50%
• Relative Magnitude 50%
• Effective Diffusivity 50%
• Blast Wave 50%
• Internal Structure 50%

Physics

• Supernovae 100%
• Superbubbles 100%
• Turbulent Mixing 16%
• Supersonics 16%
• Diffusivity 16%
• Blast Wave 16%
• Heat Conduction 16%
• Dynamical Evolution 16%
• High Temperature Gas 16%

Keyphrases

• Gas Energy 16%
• Bubble Shells 16%