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Seeding black holes in cosmological simulations
P. Taylor,
C. 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
52
Citations (Scopus)
71
Downloads (Pure)
Overview
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Keyphrases
Cosmological Simulations
100%
Dispersion Relation
66%
Star Formation
66%
Velocity Dispersion
66%
Galaxies
66%
High Density
33%
Population III Stars
33%
Order of Magnitude
33%
First Stars
33%
Density Peaks
33%
Galactic Winds
33%
Gas Accretion
33%
Surrounding Materials
33%
Star Formation Rate
33%
Massive Black Holes
33%
Physical Effects
33%
Black Hole Mass
33%
Seed Mass
33%
Active Galactic nuclei
33%
Mass Velocity
33%
Physics
Black Holes
100%
Population III Stars
28%
Star Formation
28%
Galactic Wind
14%
Star Formation Rate
14%
Active Galactic Nuclei
14%