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dc.contributor.authorUrquhart, Ryan Troy
dc.contributor.supervisorJames Miller-Jonesen_US
dc.date.accessioned2019-07-05T01:47:59Z
dc.date.available2019-07-05T01:47:59Z
dc.date.issued2018en_US
dc.identifier.urihttp://hdl.handle.net/20.500.11937/75836
dc.description.abstract

Ultraluminous X-ray sources (ULXs) represent stellar-mass binary systems accreting at extreme rates. Their observational diversity has been attributed to numerous different physical interpretations. Here we analyse multiwavelength observations of a select number of ULXs demonstrating a wide range of contrasting observable properties. We present the discovery of the first eclipsing ULXs, a detailed study of outflows, an examination of the highest accretion-rate sources, and finally, discuss how ULX observational and physical properties might be related.

en_US
dc.publisherCurtin Universityen_US
dc.titleRegimes of Super-Eddington Accretion and Outflows in Extragalactic X-ray Binariesen_US
dc.typeThesisen_US
dcterms.educationLevelPhDen_US
curtin.departmentCurtin Institute of Radio Astronomyen_US
curtin.accessStatusOpen accessen_US
curtin.facultyScience and Engineeringen_US


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