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Galaxy Core Formation by Supermassive Black Hole Binaries: The Importance of Realistic Initial Conditions and Galaxy Morphology
Fani Dosopoulou
,
Jenny E. Greene
, Chung Pei Ma
Astrophysical Sciences
Research output
:
Contribution to journal
›
Article
›
peer-review
8
Scopus citations
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Dive into the research topics of 'Galaxy Core Formation by Supermassive Black Hole Binaries: The Importance of Realistic Initial Conditions and Galaxy Morphology'. Together they form a unique fingerprint.
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Keyphrases
Galaxies
100%
Galaxy Mergers
100%
Supermassive Black Hole Binaries
100%
Core Formation
100%
Galaxy Morphology
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%
Supermassive Black Holes (SMBHs)
33%
Binding Energy
33%
Cusp
33%
Galaxy Properties
33%
Density Core
33%
Merger Simulation
33%
Radius of Influence
33%
Physics
Supermassive Black Holes
100%
Galaxy Mergers
100%
Galaxy Classification Systems
100%
Mass Ratio
66%
Stellar Mass
66%
High Resolution
33%
Elliptical Galaxy
33%
Monte Carlo
33%
Binding Energy
33%
Galaxy Properties
33%