Detection of Giant Pulses from the Pulsar PSR B0031-07

Details Detection of Giant Pulses from the Pulsar PSR B0031-07 Detection of Giant Pulses from the Pulsar PSR B0031-07

2004-02-18

arxiv.org/abs/astro-ph/0402425v1

Astron.Lett. 30 (2004) 247-250

Astronomy and Astrophysics

Astrophysics

7 pages, 2 figures, to appear in: Pis'ma v Astronomicheskii Zhurnal, 2004, v.30, No.4, and will be translated as: Astronomy Le

Scientific paper

10.1134/1.1695085

Giant pulses have been detected from the pulsar PSR B0031-07. A pulse with an intensity higher than the intensity of the average pulse by a factor of 50 or more is encountered approximately once per 300 observed periods. The peak flux density of the strongest pulse is 530 Jy, which is a factor of 120 higher than the peak flux density of the average pulse. The giant pulses are a factor of 20 narrower than the integrated profile and are clustered about its center.

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