Giant Pulses in Pulsar PSR J1752+2359

2006/05/03 by А. А. Ершов, A. A. Ershov, Ershov, A. A. +3
Earth and Planetary Sciences · Engineering · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #High-pressure geophysics and materials #Pulsars and Gravitational Waves Research #Superconducting Materials and Applications #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0605086

5 pages, 4 figures, to appear in Chin. J. Astron. Astrophys, proceedings of The 2005 Lake Hanas International Pulsar Symposium

arxiv created 2006/05/03 · openalex publication_date 2006/05/03 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

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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