Detection of Giant Pulses from the Pulsar PSR B1112+50

Details Detection of Giant Pulses from the Pulsar PSR B1112+50 Detection of Giant Pulses from the Pulsar PSR B1112+50

2002-12-23

arxiv.org/abs/astro-ph/0212529v1

Astron.Lett. 29 (2003) 91-95; Pisma Astron.Zh. 29 (2003) 111-115

Astronomy and Astrophysics

Astrophysics

5 pages, 4 figures, to appear in: Pis'ma v Astronomicheskii Zhurnal, 2003, v.29, No.2, p111-115 and will be translated as: Ast

Scientific paper

10.1134/1.1544530

We detected giant pulses from the pulsar PSR B1112+50. A pulse with an intensity that is a factor of 30 or more higher than the intensity of the average pulse is encountered approximately once in 150 observed pulses. The peak .ux density of the strongest pulse is about 180 Jy. This value is a factor of 80 higher than the peak .ux density of the average pulse. The giant pulses are narrower than the average prfile approximately by a factor of 5 and they cluster about the center of the average profile.

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