Arecibo Measurements of Pulsar--White Dwarf Binaries: Evidence for Heavy Neutron Stars

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dc.creatorNice, David J.
dc.creatorSplaver, Eric M.
dc.creatorStairs, Ingrid H.
dc.date2004-11-08
dc.date.accessioned2026-07-07T02:15:42Z
dc.date.available2026-07-07T02:15:42Z
dc.descriptionWe summarize constraints on neutron star masses from ongoing timing observations of pulsar-white dwarf binaries at Arecibo. The trend is toward pulsar masses larger than the canonical value of 1.35 solar masses.
dc.description2 pages, to appear in "Binary Radio Pulsars", eds F. A. Rasio & I. H. Stairs, PASP conf series
dc.identifierhttps://arxiv.org/abs/astro-ph/0411207
dc.identifierhttp://arxiv.org/abs/astro-ph/0411207
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8508
dc.subjectAstrophysics
dc.titleArecibo Measurements of Pulsar--White Dwarf Binaries: Evidence for Heavy Neutron Stars
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