Determination of the orbital parameters of binary pulsars

dc.creatorFreire, P. C.
dc.creatorKramer, M.
dc.creatorLyne, A. G.
dc.date2000-10-23
dc.date.accessioned2026-07-07T11:28:44Z
dc.date.available2026-07-07T11:28:44Z
dc.descriptionWe present a simple novel method for determining the orbital parameters of binary pulsars. This method works with any sort of orbital sampling, no matter how sparse, provided that information on the period derivatives is available with each measurement of the rotational period of the pulsar, and it is applicable to binary systems with nearly circular orbits. We use the technique to precisely estimate the hitherto unknown orbital parameters of two binary millisecond pulsars in the globular cluster 47 Tucanae, 47 Tuc S and T. The method can also be used more generally to make first-order estimates of the orbital parameters of binary systems using a minimal amount of data.
dc.description13 pages, 6 figures, accepted for publication in MNRAS
dc.identifierhttps://arxiv.org/abs/astro-ph/0010463
dc.identifierhttp://arxiv.org/abs/astro-ph/0010463
dc.identifierMon.Not.Roy.Astron.Soc.322:885,2001
dc.identifierdoi:10.1046/j.1365-8711.2001.04200.x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196490
dc.subjectAstrophysics
dc.titleDetermination of the orbital parameters of binary pulsars
dc.typetext

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