The double pulsar -- A new testbed for relativistic gravity

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dc.creatorKramer, M.
dc.creatorLyne, A. G.
dc.creatorBurgay, M.
dc.creatorPossenti, A.
dc.creatorManchester, R. N.
dc.creatorCamilo, F.
dc.creatorMcLaughlin, M. A.
dc.creatorLorimer, D. R.
dc.creatorD'Amico, N.
dc.creatorJoshi, B. C.
dc.creatorReynolds, J.
dc.creatorFreire, P. C. C.
dc.date2004-05-10
dc.date.accessioned2026-07-07T02:13:09Z
dc.date.available2026-07-07T02:13:09Z
dc.descriptionThe first ever double pulsar, discovered by our team a few months ago, consists of two pulsars, one with period of 22 ms and the other with a period of 2.7 s. This binary system with a period of only 2.4-hr provides a truly unique laboratory for relativistic gravitational physics. In this contribution we summarize the published results and look at the prospects of future observations.
dc.description6 pages, two figures, to appear in "Binary Pulsars" Eds. Rasio & Stairs, PASP
dc.identifierhttps://arxiv.org/abs/astro-ph/0405179
dc.identifierhttp://arxiv.org/abs/astro-ph/0405179
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7712
dc.subjectAstrophysics
dc.titleThe double pulsar -- A new testbed for relativistic gravity
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