Detection of Giant Pulses in Pulsar PSR J1752+2359

Details Detection of Giant Pulses in Pulsar PSR J1752+2359 Detection of Giant Pulses in Pulsar PSR J1752+2359

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006chjas...6b..30e&link_type=abstract

Chinese Journal of Astronomy and Astrophysics, Supplement, Volume 6, Issue S2, Proceedings of the 2005 Lake Hanas International

Astronomy and Astrophysics

Astrophysics

Stars: Neutron, Pulsars: General, Pulsars: Individual Psr J1752+2359

Scientific paper

We report the detection of Giant Pulses (GPs) in the pulsar PSR J1752+2359. The energy of the strongest GP exceeds the energy of the average pulse by a factor of 200, in which it stands out from all known pulsars with GPs. PSR J1752+2359 as well as the previously detected PSR B0031-07 and PSR B1112+50, belongs to the first group of pulsars found to have GPs without a high magnetic field at the light cylinder.

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