Investigating the Links between Radio Pulsar Populations that Display Intermittent Emission Phenomena at Low Frequencies
dc.contributor.author | Meyers, Bradley Ward | |
dc.contributor.supervisor | Ramesh Bhat | en_US |
dc.date.accessioned | 2019-08-27T08:08:30Z | |
dc.date.available | 2019-08-27T08:08:30Z | |
dc.date.issued | 2019 | en_US |
dc.identifier.uri | http://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.publisher | Curtin University | en_US |
dc.title | Investigating the Links between Radio Pulsar Populations that Display Intermittent Emission Phenomena at Low Frequencies | en_US |
dc.type | Thesis | en_US |
dcterms.educationLevel | PhD | en_US |
curtin.department | Physics and Astronomy | en_US |
curtin.accessStatus | Open access | en_US |
curtin.faculty | Science and Engineering | en_US |