Abstract
The goal of my thesis is to model the merging timescale of galaxies in N-body simulations and provide an analytical formula that can be applied in galaxy formation models. I assessed the algorithms used to identify and track simulated mergers using a new visualisation tool, the dendogram. I then quantified how merger timescales depend on galaxy orbits and compared to predictions from prescriptions in the literature. Finally, I used these insights to develop a new model for the merger timescale, showing how it improves on existing prescriptions, and explored its implications for predictions in the semi-analytical galaxy formation model, Shark.
| Original language | English |
|---|---|
| Qualification | Doctor of Philosophy |
| Awarding Institution |
|
| Supervisors/Advisors |
|
| Thesis sponsors | |
| Award date | 2 Aug 2020 |
| DOIs | |
| Publication status | Unpublished - 2020 |