Detection of Giant Pulses in pulsar PSR J1752+2359

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dc.creatorErshov, A. A.
dc.creatorKuzmin, A. D.
dc.date2005-09-04
dc.date.accessioned2026-07-07T06:28:51Z
dc.date.available2026-07-07T06:28:51Z
dc.descriptionWe report the detection of Giant Pulses (GPs) in the pulsar PSR J1752+2359. About one pulse in 270 has a peak flux density more than 40 times the peak flux density of an average pulse (AP), and the strongest GP is as large as 260. The energy of the strongest GP exceeds the energy of the average pulse by a factor of 200 which is greater than in other known pulsars with GPs. PSR J1752+2359 as well as the previously detected pulsars PSR B0031-07 and PSR B1112+50, belong to the first group of pulsars found to have GPs without a strong magnetic field at the light cylinder.
dc.description5 pages, 4 figures, 1 table. Accepted for publication in A&A
dc.identifierhttps://arxiv.org/abs/astro-ph/0509068
dc.identifierhttp://arxiv.org/abs/astro-ph/0509068
dc.identifierAstron.Astrophys. 443 (2006) 593
dc.identifierdoi:10.1051/0004-6361:20052790
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/97841
dc.subjectAstrophysics
dc.titleDetection of Giant Pulses in pulsar PSR J1752+2359
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