Large-scale galactic turbulence: Can self-gravity drive the observed H i velocity dispersions?

Keyphrases

• Velocity Dispersion 100%
• Galactic 100%
• Star Formation Rate 100%
• Turbulence 100%
• Self-gravity 100%
• Gravity-driven 100%
• Galaxies 66%
• Gaseous Phase 66%
• Dispersion Profile 66%
• High-resolution 33%
• Star Formation 33%
• Dark Matter Halos 33%
• Disk Galaxies 33%
• Self-gravitating 33%
• Thermal Instability 33%
• Baryons 33%
• Supernovae 33%
• Galactic Disks 33%
• Gravitational Instability 33%
• Large Population 33%
• Multiphase Media 33%
• Turbulent Motion 33%
• Individual-galaxies 33%
• Turbulent Velocity 33%
• Shearing Motion 33%
• Formation Feedback 33%
• Cold Cloud 33%
• Shock Heating 33%
• Non-axisymmetric Mode 33%
• Area 10 33%
• Tidal Interactions 33%
• Adaptive Mesh Simulation 33%

Physics

• Star Formation Rate 100%
• High Resolution 33%
• Dark Matter 33%
• Star Formation 33%
• Disk Galaxy 33%
• Thermal Instability 33%
• Baryon 33%
• Supernovae 33%
• Gravitational Instability 33%
• Shock Heating 33%
• Tidal Interaction 33%