Full description
CU Virginis is the best-studied member of the class of stellar radio transients known as stellar pulsars. Its circularly polarised radio pulses are explained by a model, which has consequences for the frequency-time dependence, polarisation and spectra of the pulses which can be tested using the Parkes ultra-wide-bandwidth receiver system. We propose to perform these tests and to demonstrate that the Parkes telescope can be used to observe transient events on time scales of minutes to hours.Available: 2021-10-03
Data time period: 2021-04-01 to 2021-09-30
Subjects
Astronomical Sciences |
Astronomical Sciences Not Elsewhere Classified |
Physical Sciences |
neutron stars |
pulsars |
transients |
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Identifiers
- DOI : 10.25919/18QT-4M38
- Handle : 102.100.100/430249
- URL : data.csiro.au/collection/csiro:52579
