The Distribution of Cool Gas In and Around Galaxies
| Field | Value | Language |
| dc.contributor.author | Weng, Simon | |
| dc.date.accessioned | 2024-08-20T23:19:02Z | |
| dc.date.available | 2024-08-20T23:19:02Z | |
| dc.date.issued | 2024 | en_AU |
| dc.identifier.uri | https://hdl.handle.net/2123/32970 | |
| dc.description.abstract | Unraveling the evolutionary paths of galaxies remains a key focus in astronomy. Over the past decade, the circumgalactic medium (CGM) has been recognised as a pivotal component in this research, serving as a record keeper of the processes of accretion and outflows, which move gas to and from the interstellar medium. In this thesis, we explore the CGM properties of galaxies, linking these properties to their stellar properties and using simulations to guide the interpretation of the observational findings. | en_AU |
| dc.language.iso | en | en_AU |
| dc.subject | Astronomy | en_AU |
| dc.subject | Astrophysics | en_AU |
| dc.subject | Galaxy Evolution | en_AU |
| dc.subject | Quasar | en_AU |
| dc.subject | Circumgalactic Medium | en_AU |
| dc.title | The Distribution of Cool Gas In and Around Galaxies | en_AU |
| dc.type | Thesis | |
| dc.type.thesis | Doctor of Philosophy | en_AU |
| dc.rights.other | The author retains copyright of this thesis. It may only be used for the purposes of research and study. It must not be used for any other purposes and may not be transmitted or shared with others without prior permission. | en_AU |
| usyd.faculty | SeS faculties schools::Faculty of Science::School of Physics | en_AU |
| usyd.degree | Doctor of Philosophy Ph.D. | en_AU |
| usyd.awardinginst | The University of Sydney | en_AU |
| usyd.advisor | Sadler, Elaine |
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