Young Pulsars from the Parkes Multibeam Pulsar Survey and their Associations

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dc.creatorManchester, R. N.
dc.creatorBell, J. F.
dc.creatorCamilo, F.
dc.creatorKramer, M.
dc.creatorLyne, A. G.
dc.creatorHobbs, G. B.
dc.creatorJoshi, B. C.
dc.creatorCrawford, F.
dc.creatorD'Amico, N.
dc.creatorPossenti, A.
dc.creatorKaspi, V. M.
dc.creatorStairs, I. H.
dc.date2001-12-07
dc.date2001-12-08
dc.date.accessioned2026-07-07T02:01:44Z
dc.date.available2026-07-07T02:01:44Z
dc.descriptionThe Parkes multibeam pulsar survey is covering a 10deg-wide strip of the southern Galactic plane from l=260deg to l=50deg. It utilizes a 13-beam receiver operating in the 20-cm band on the Parkes 64-m radio telescope and is much more sensitive than any previous large-scale survey. Most of the 608 pulsars discovered so far are relatively distant and many are young, with 37 having a characteristic age of less than 10^5 years. At least one of these is associated with a supernova remnant and four other probable associations are suggested. Several multibeam pulsars have high values of the parameter Edot/d^2 and are within the position error contours of unidentified EGRET gamma-ray sources. These possible associations will be tested with the advent of new gamma-ray telescopes.
dc.description6 pages, 2 figs. To appear in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P.O.Slane and B.M.Gaensler
dc.identifierhttps://arxiv.org/abs/astro-ph/0112166
dc.identifierhttp://arxiv.org/abs/astro-ph/0112166
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3860
dc.subjectAstrophysics
dc.titleYoung Pulsars from the Parkes Multibeam Pulsar Survey and their Associations
dc.typetext

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