From seed to supermassive: simulating the origin, evolution and impact of massive black holes
<p>First observed as early as redshift z = 7 and now thought to be found at the centre of every massive galaxy in the local Universe, the evolution history of supermassive black holes (SMBHs) spans over 13 billion years. In this thesis, the coevolution between SMBHs and their host galaxies is...
Hovedforfatter: | Beckmann, R |
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Andre forfattere: | Devriendt, J |
Format: | Thesis |
Sprog: | English |
Udgivet: |
2017
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Fag: |
Lignende værker
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Origin of an orbiting star around the galactic supermassive black hole
af: Shogo NISHIYAMA, et al.
Udgivet: (2023-12-01) -
Direct Formation of Massive Black Holes via Dynamical Collapse in Metal-enriched Merging Galaxies at z ∼ 10: Fully Cosmological Simulations
af: Lucio Mayer, et al.
Udgivet: (2024-01-01) -
Black hole binary formation and mergers in supermassive black hole discs
af: Rowan, C
Udgivet: (2024) -
The Hydrodynamic Evolution of Binary Black Holes Embedded within the Vertically Stratified Disks of Active Galactic Nuclei
af: Nicholas Kaaz, et al.
Udgivet: (2023-01-01) -
Growth of a Massive Black Hole in a Dense Star Cluster Via Tidal Disruption Accretion
af: Seungjae Lee, et al.
Udgivet: (2023-01-01)