Twenty Years of Searching for (and Finding) Globular Cluster Pulsars

dc.creatorRansom, Scott M.
dc.date2007-10-19
dc.date.accessioned2026-07-07T11:12:24Z
dc.date.available2026-07-07T11:12:24Z
dc.descriptionGlobular clusters produce orders of magnitude more millisecond pulsars per unit mass than the Galactic disk. Since the first cluster pulsar was uncovered twenty years ago, at least 138 have been identified - most of which are binary millisecond pulsars. Because of their origins involving stellar encounters, many of these systems are exotic objects that would never be observed in the Galactic disk. Examples include pulsar-main sequence binaries, extremely rapid rotators (including the current record holder), and millisecond pulsars in highly eccentric orbits. These systems are allowing new probes of the interstellar medium, the equation of state of material at supra-nuclear density, the mass distribution of neutron stars, and the dynamics of globular clusters.
dc.description9 pages, 6 figures. Submitted review for the "40 Years of Pulsars" conference in Montreal, Aug 2007. To be published by the AIP
dc.identifierhttps://arxiv.org/abs/0710.3626
dc.identifierhttp://arxiv.org/abs/0710.3626
dc.identifierAIPConf.Proc.983:415-423,2008
dc.identifierdoi:10.1063/1.2900267
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191369
dc.subjectAstrophysics
dc.titleTwenty Years of Searching for (and Finding) Globular Cluster Pulsars
dc.typetext

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