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dc.contributor.authorTudor, Vlad Andrei
dc.contributor.supervisorJames Miller-Jonesen_US
dc.date.accessioned2019-07-05T03:21:50Z
dc.date.available2019-07-05T03:21:50Z
dc.date.issued2018en_US
dc.identifier.urihttp://hdl.handle.net/20.500.11937/75837
dc.description.abstract

Globular clusters host a myriad of dynamically-formed objects, some of which may be black hole X-ray binaries. The existence of such systems in globular clusters has yet to be confirmed, but deep radio observations may efficiently find them. The MAVERIC survey was conceived with this goal in mind. In this thesis I present its results, highlighting black hole candidates, contrasting them with neutron star systems, and gauging their nature.

en_US
dc.publisherCurtin Universityen_US
dc.titleThe Radio Source Population of Globular Clustersen_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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