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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2698
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dc.contributor.authorDatta, B-
dc.contributor.authorAlpar, M. A-
dc.date.accessioned2008-07-16T06:01:50Z-
dc.date.available2008-07-16T06:01:50Z-
dc.date.issued1993-08-
dc.identifier.citationAstronomy and Astrophysics , Vol. 275, No. 1, pp. 210 - 212en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/2698-
dc.description.abstractThe dynamical models for neutron star glitches and postglitch behaviour, and the information they yield on the crustal moment of inertia, are applied to a catalogue of neutron star models. The implications for neutron star equations of state are discussed. The postglitch timing data from the Vela pulsar are interpreted to rule out one of the softer equations of state for neutron matter with an admixture of hypersons, if the neutron star mass is 1.4 solar mass.en
dc.format.extent501305 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEuropean Southern Observatoryen
dc.relation.urihttp://adsabs.harvard.edu/abs/1993A%26A...275..210Den
dc.subjectNeutron star: equation of stateen
dc.subjectNeutron star: glitchesen
dc.titleImplications of the Crustal Moment of Inertia for Neutron Star Equations of Stateen
dc.typeArticleen
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