Timing the Parkes Multibeam Pulsars

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dc.creatorManchester, R. N.
dc.creatorLyne, A. G.
dc.creatorCamilo, F.
dc.creatorKaspi, V. M.
dc.creatorStairs, I. H.
dc.creatorCrawford, F.
dc.creatorMorris, D. J.
dc.creatorBell, J. F.
dc.creatorD'Amico, N.
dc.date1999-11-16
dc.date1999-11-17
dc.date.accessioned2026-07-07T02:34:30Z
dc.date.available2026-07-07T02:34:30Z
dc.descriptionMeasurement of accurate positions, pulse periods and period derivatives is an essential follow-up to any pulsar survey. The procedures being used to obtain timing parameters for the pulsars discovered in the Parkes multibeam pulsar survey are described. Completed solutions have been obtained so far for about 80 pulsars. They show that the survey is preferentially finding pulsars with higher than average surface dipole magnetic fields. Eight pulsars have been shown to be members of binary systems and some of the more interesting results relating to these are presented.
dc.description6 pages, 2 embedded EPS figures, to be published in proceedings of "Pulsar Astronomy - 2000 and Beyond", ASP Conf. Ser
dc.identifierhttps://arxiv.org/abs/astro-ph/9911319
dc.identifierhttp://arxiv.org/abs/astro-ph/9911319
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15266
dc.subjectAstrophysics
dc.titleTiming the Parkes Multibeam Pulsars
dc.typetext

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