Giant pulses in Millisecond Pulsars

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dc.creatorJoshi, B. C.
dc.creatorKramer, M.
dc.creatorLyne, A. G.
dc.creatorMclaughlin, M.
dc.creatorStairs, I. H.
dc.date2003-10-10
dc.date.accessioned2026-07-07T02:10:18Z
dc.date.available2026-07-07T02:10:18Z
dc.descriptionGiant 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).
dc.description2 pages, 2 figures, To appear in "Young Neutron Stars and Their Environments"(IAU Symposium 218, ASP Conference Proceedings), eds F. Camilo and B. M. Gaensler
dc.identifierhttps://arxiv.org/abs/astro-ph/0310285
dc.identifierhttp://arxiv.org/abs/astro-ph/0310285
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6694
dc.subjectAstrophysics
dc.titleGiant pulses in Millisecond Pulsars
dc.typetext

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