Pulsar transient radio emission

Details Pulsar transient radio emission Pulsar transient radio emission

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..968..159l&link_type=abstract

ASTROPHYSICS OF COMPACT OBJECTS: International Conference on Astrophysics of Compact Objects. AIP Conference Proceedings, Volum

Astronomy and Astrophysics

Astrophysics

Pulsars, Neutron Stars, Radiation Mechanisms, Polarization

Scientific paper

Radiation processes in the closed field line regions of pulsar magnetospheres are discussed. It is argued that trapped particles form radiation belts in the closed field line regions in the majority of pulsars. It is proposed that transient radio emission, seen as rotating radio transients (RRATs), results from events that trigger precipitation of these trapped particles.

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