Modeling high-redshift galaxies: What can we learn from high and ultra-high resolution hydrodynamical simulations?

Keyphrases

• Milky Way 100%
• Hydrodynamic Simulation 100%
• Ultra-high Resolution 100%
• High-redshift Galaxies 100%
• High-resolution 50%
• Dust 50%
• Galaxies 50%
• Star Formation 50%
• Blowing 50%
• Luminosity Function 50%
• Cosmology 50%
• Cosmological Parameters 50%
• Cold Gas 50%
• Globular Clusters 50%
• Existing Data 50%
• Dust Extinction 50%
• Galaxy Formation 50%
• Ultra-high 50%
• Thin Disk 50%
• Galactic Winds 50%
• Re-simulation 50%
• Mare Nostrum 50%

Physics

• High Resolution 100%
• Milky Way 100%
• Hydrodynamical Simulations 100%
• High-Redshift Galaxy 100%
• Protogalaxies 100%
• Star Formation 50%
• Luminosity Function 50%
• Cosmological Parameters 50%
• Globular Cluster 50%
• Galactic Evolution 50%
• Cold Gas 50%
• Galactic Wind 50%