Galaxy Core Formation by Supermassive Black Hole Binaries: The Importance of Realistic Initial Conditions and Galaxy Morphology

Keyphrases

• Galaxies 100%
• Galaxy Mergers 100%
• Core Formation 100%
• Galaxy Morphology 100%
• Supermassive Black Hole Binary 100%
• Mass Ratio 66%
• Stellar Masses 66%
• Range of Values 33%
• High-resolution 33%
• Monte Carlo Method 33%
• Low Density 33%
• Order of Magnitude 33%
• Elliptical Galaxies 33%
• Core Size 33%
• N-body 33%
• Binding Energy 33%
• Cusp 33%
• Galaxy Properties 33%
• Density Core 33%
• Merger Simulation 33%
• Radius of Influence 33%
• Supermassive Black Hole (SMBH) 33%
• Merger History 33%

Physics

• Supermassive Black Holes 100%
• Galaxy Mergers 100%
• Galaxy Classification Systems 100%
• Mass Ratio 66%
• Stellar Mass 66%
• High Resolution 33%
• Monte Carlo 33%
• Binding Energy 33%
• Galaxy Properties 33%
• Elliptical Galaxy 33%