Full description
We propose to observe the magnetars 1E 1547.0-5408 and PSR J1622-4950\rapproximately weekly, to track their rotation, flux density, and\r
polarisation, as we have been doing through this project. Also, as\r
of late 2018, XTE J1810-197 is again a radio magnetar after 10 years\r
dormant! Its chaotic rotation is better tracked in detail elsewhere,\r
but weekly observations with the UWL receiver are already providing\r
unique measurements of its radio spectrum and broad-band behaviour.\r
Our observations provide an important window into remarkably dynamic\r
magnetar magnetospheres, and characterise the conditions under which\r
radio emission takes place therein, placing constraints on the\r
emission mechanisms, which in at least some significant respects\r
differ from those of ordinary pulsars.
Available: 2020-03-23
Data time period: 2019-10-01 to 2020-03-31
Subjects
Astronomical Sciences |
Astronomical Sciences Not Elsewhere Classified |
P885_2019OCTS |
Physical Sciences |
neutron stars |
pulsars |
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Identifiers
- DOI : 10.25919/5E777CE5D8DF4
- Handle : 102.100.100/340624
- URL : data.csiro.au/collection/csiro:43583
