Neutron Star Masses from Arecibo Timing Observations of Five Pulsar-White Dwarf Binary Systems

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dc.creatorNice, David J.
dc.creatorSplaver, Eric M.
dc.creatorStairs, Ingrid H.
dc.date2002-10-29
dc.date.accessioned2026-07-07T02:05:53Z
dc.date.available2026-07-07T02:05:53Z
dc.descriptionWe have detected relativistic and/or kinematic post-Keplerian parameters of no fewer than five pulsar-white dwarf binary systems in long-term timing observations at Arecibo. We discuss the resulting constraints on pulsar and companion masses. The general trend is that the pulsar mass measurements are compatible with the canonical value of 1.35 solar masses, but in most cases somewhat higher masses are preferred.
dc.description6 pages, to appear in proceedings of "Radio Pulsars," Chania, Crete, August 2002 (ASP conference series)
dc.identifierhttps://arxiv.org/abs/astro-ph/0210637
dc.identifierhttp://arxiv.org/abs/astro-ph/0210637
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5242
dc.subjectAstrophysics
dc.titleNeutron Star Masses from Arecibo Timing Observations of Five Pulsar-White Dwarf Binary Systems
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