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Time Evolution of Galaxy Scaling Relations in Cosmological Simulations
Philip Taylor,
Chiaki Kobayashi
Centre for Astrophysics Research (CAR)
School of Physics, Engineering & Computer Science
Department of Physics, Astronomy and Mathematics
Research output
:
Contribution to journal
›
Article
›
peer-review
33
Citations (Scopus)
81
Downloads (Pure)
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Dive into the research topics of 'Time Evolution of Galaxy Scaling Relations in Cosmological Simulations'. Together they form a unique fingerprint.
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Keyphrases
AGN Feedback
66%
Black Hole Mass
33%
Chemical Evolution
33%
Cosmological Hydrodynamical Simulation
33%
Cosmological Simulations
100%
Dispersion Relation
33%
Galaxies
100%
Galaxy Evolution
100%
Galaxy Masses
33%
Galaxy Scaling Relations
100%
Gas Phase
33%
High-redshift
33%
Main Sequence
33%
Mass Size
33%
Mass Velocity
33%
Massive Galaxies
33%
Metallicity
100%
Scaling Relations
33%
Scaling Relationship
33%
SIM1
33%
SIM2
33%
Size Relationship
33%
Star Formation
33%
Steep Slope
33%
Stellar Masses
33%
Velocity Dispersion
33%
Physics
Active Galactic Nuclei
66%
Black Holes
100%
Chemical Evolution
33%
Galaxy Evolution
100%
Galaxy Masses
33%
Hydrodynamical Simulations
33%
Metallicity
100%
Star Formation
33%
Stellar Mass
33%
Vapor Phase
33%