Thesis
Characterising filaments in cosmological simulations
- Abstract:
-
At high redshift, the cosmic web is widely expected to have a significant impact on the morphologies, dynamics and star formation rates of the galaxies embedded within it, underscoring the need for a comprehensive study of the properties of such a filamentary network. With this goal in mind, we perform an analysis of high-z gas and dark matter (DM) filaments around a Milky Waylike progenitor simulated with the RAMSES adaptive mesh refinement (AMR) code from cosmic scales (∼1 Mpc) down...
Expand abstract
Actions
Access Document
- Files:
-
-
(Preview, Dissemination version, pdf, 23.8MB, Terms of use)
-
Authors
Contributors
+ Slyz, A
- Role:
- Supervisor
+ Devriendt, J
- Role:
- Supervisor
+ Lintott, C
- Role:
- Examiner
- ORCID:
- 0000-0001-5578-359X
+ Pichon, C
- Role:
- Examiner
+ Science and Technology Facilities Council
More from this funder
- Funder identifier:
- http://dx.doi.org/10.13039/501100000271
- Grant:
- 10.13039/501100000271
- DOI:
- Type of award:
- DPhil
- Level of award:
- Doctoral
- Awarding institution:
- University of Oxford
- Language:
-
English
- Keywords:
- Subjects:
- Deposit date:
-
2021-03-15
- ARK identifier:
Terms of use
- Copyright holder:
- Ramsøy, M
- Copyright date:
- 2020
If you are the owner of this record, you can report an update to it here: Report update to this record