The Distribution of Cool Gas In and Around Galaxies

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Open Access

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
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
dc.language.iso	en	en
dc.subject	Astronomy	en
dc.subject	Astrophysics	en
dc.subject	Galaxy Evolution	en
dc.subject	Quasar	en
dc.subject	Circumgalactic Medium	en
dc.title	The Distribution of Cool Gas In and Around Galaxies	en
dc.type	Thesis
dc.type.thesis	Doctor of Philosophy	en
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
usyd.faculty	SeS faculties schools::Faculty of Science::School of Physics	en
usyd.degree	Doctor of Philosophy Ph.D.	en
usyd.awardinginst	The University of Sydney	en
usyd.advisor	Sadler, Elaine