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dc.contributor.authorRussell, Thomas David
dc.contributor.supervisorDr Peter Curran
dc.contributor.supervisorDr James Miller-Jones
dc.contributor.supervisorProf. Steven Tingay
dc.contributor.supervisorDr Roberto Soria
dc.date.accessioned2017-01-30T09:58:28Z
dc.date.available2017-01-30T09:58:28Z
dc.date.created2015-09-18T06:04:29Z
dc.date.issued2015
dc.identifier.urihttp://hdl.handle.net/20.500.11937/1080
dc.description.abstract

This thesis presents multiwavelength monitoring of the Galactic black hole candidate X-ray binary MAXI J1836-194 during its 2011 outburst. The observations have been used to probe the relationship between the inflow and outflow around this accreting stellar-mass black hole with unprecedented detail, delivering new information on the evolution of the accretion and ejection processes and how they are coupled, providing insight into how accretion-powered jets are launched on all physical scales.

dc.languageen
dc.publisherCurtin University
dc.titleThe connection between inflow and outflow around accreting stellar-mass black holes
dc.typeThesis
dcterms.educationLevelPhD
curtin.departmentSchool of ScienceDepartment of Physics & Astronomy
curtin.accessStatusOpen access


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