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27 April 2024 |
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The double pulsar -- A new testbed for relativistic gravity | | M. Kramer
; A.G. Lyne
; M. Burgay
; A. Possenti
; R.N. Manchester
; F. Camilo
; M.A. McLaughlin
; D.R. Lorimer
; N. D’Amico
; B.C. Joshi
; J. Reynolds
; P.C.C. Freire
; | | Date: |
10 May 2004 | | Subject: | astro-ph | | Affiliation: | 3,4), R.N. Manchester , F. Camilo , M.A. McLaughlin , D.R. Lorimer , N. D’Amico (4,7), B.C. Joshi , J. Reynolds , P.C.C. Freire , (1-University of Manchester, Jodrell Bank Observatory) (2-Universita degli Studi di Bologna), (3-INAF - Osservatori | | Abstract: | The 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. | | Source: | arXiv, astro-ph/0405179 | | Services: | Forum | Review | PDF | Favorites | |
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