Brief description
Understanding rotating radio transients (RRATs) has the potential to uproot our understanding of core-collapse supernovae and the overall evolution of neutron stars. Despite this, RRATs remain an enigma and has numerous potential and conflicting explanations in the literature. These observations will observe a sample of RRATs with the UWL receiver, in tandem with the Five-hundred-meter Aperture Spherical Telescope (FAST), in order to directly test many of the competing theories that exist around RRATs and answer the question of where they fit amongst the overall population of neutron stars.Data time period: 2019-04-01 to 2019-09-30
Subjects
Astronomical and Space Sciences |
Astronomical and Space Sciences Not Elsewhere Classified |
Physical Sciences |
pulsars, neutron stars, transients, P1016_2019APRS |
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Identifiers
- Local : 102.100.100/143599
- DOI : 10.25919/5d3042fd3374d