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dc.contributor.authorMeyers, Bradley Ward
dc.contributor.supervisorRamesh Bhaten_US
dc.date.accessioned2019-08-27T08:08:30Z
dc.date.available2019-08-27T08:08:30Z
dc.date.issued2019en_US
dc.identifier.urihttp://hdl.handle.net/20.500.11937/76186
dc.description.abstract

Pulsars are unparalleled astrophysical tools, yet, after more than 50 years of research, we still do not fully understand the mechanism responsible for their radio emission. Through a series of systematic, simultaneous and wideband observations of three sporadically emitting pulsars, we have revealed the importance of low-frequency information when characterising the emission, and support the idea that the intermittent emission behaviour is likely due to the same physical mechanism operating on different time scales.

en_US
dc.publisherCurtin Universityen_US
dc.titleInvestigating the Links between Radio Pulsar Populations that Display Intermittent Emission Phenomena at Low Frequenciesen_US
dc.typeThesisen_US
dcterms.educationLevelPhDen_US
curtin.departmentPhysics and Astronomyen_US
curtin.accessStatusOpen accessen_US
curtin.facultyScience and Engineeringen_US


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