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20 April 2024
 
  » arxiv » astro-ph/0310285

 Article overview


Giant pulses in Millisecond Pulsars
B. C. Joshi ; M. Kramer ; A. G. Lyne ; M. Mclaughlin ; I. H. Stairs ;
Date 10 Oct 2003
Subject astro-ph
Affiliation1 and 2), M. Kramer , A. G. Lyne , M. Mclaughlin , I. H. Stairs ( National Center for Radio Astrophysics, Pune, India, Jodrell Bank Observatory, University of Manchester, Macclesfield, UK, University of British Columbia, Vancouver, Canada
AbstractGiant pulses (GPs), occasional individual pulses with an intensity 100 times the average intensity, have been detected in four pulsars todate. Their origin is not well understood, but studies suggest a connection between the strength of magnetic field at the light cylinder B_lc and the existence of GPs. Here, we report on detection of significant Large Amplitude Pulses (LAPs) in two more pulsars with high values of B_lc, PSRs J0218+4232 and B1957+20, observed using Giant Meterwave Radio Telescope (GMRT).
Source arXiv, astro-ph/0310285
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