Volume 443, Number 2, November IV 2005
|Page(s)||593 - 597|
|Section||Stellar structure and evolution|
|Published online||04 November 2005|
Detection of giant pulses in pulsar PSR J1752+2359
Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute, Russian Academy of Sciences, Pushchino 142290, Russia e-mail: email@example.com
2 Isaac Newton Institute, Chile, Pushchino Branch, Russia
Accepted: 20 July 2005
We 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.
Key words: stars: neutron / stars: pulsars: general / stars: pulsars: individual: PSR J1752+2359
© ESO, 2005
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.