The High Time Resolution Universe Pulsar Survey - XIII. PSR J1757-1854, the most accelerated binary pulsar

被引:64
|
作者
Cameron, A. D. [1 ]
Champion, D. J. [1 ]
Kramer, M. [1 ,2 ]
Bailes, M. [3 ,4 ,5 ]
Barr, E. D. [1 ]
Bassa, C. G. [6 ]
Bhandari, S. [3 ,4 ]
Bhat, N. D. R. [4 ,7 ]
Burgay, M. [8 ]
Burke-Spolaor, S. [9 ,10 ]
Eatough, R. P. [1 ]
Flynn, C. M. L. [3 ]
Freire, P. C. C. [1 ]
Jameson, A. [3 ,4 ]
Johnston, S. [11 ]
Karuppusamy, R. [1 ]
Keith, M. J. [2 ]
Levin, L. [2 ]
Lorimer, D. R. [9 ]
Lyne, A. G. [2 ]
McLaughlin, M. A. [9 ]
Ng, C. [12 ]
Petroff, E. [6 ]
Possenti, A. [8 ]
Ridolfi, A. [1 ]
Stappers, B. W. [2 ]
van Straten, W. [3 ,4 ,13 ]
Tauris, T. M. [1 ,14 ]
Tiburzi, C. [1 ,15 ]
Wex, N. [1 ]
机构
[1] Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
[2] Univ Manchester, Jodrell Bank Ctr Astrophys, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England
[3] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Mail H39,POB 218, Hawthorn, Vic 3122, Australia
[4] Swinburne Univ Technol, ARC Ctr Excellence All Sky Astron CAASTRO, Mail H30,POB 218, Hawthorn, Vic 3122, Australia
[5] Swinburne Univ Technol, ARC Ctr Excellence Gravitat Wave Discovery OzGrav, Mail H11,POB 218, Hawthorn, Vic 3122, Australia
[6] ASTRON, Postbus 2, NL-7990 AA Dwingeloo, Netherlands
[7] Curtin Univ, Int Ctr Radio Astron Res, Bentley, WA 6102, Australia
[8] Osservatorio Astron Cagliari, INAF, Via Sci 5, I-09047 Selargius, CA, Italy
[9] West Virginia Univ, Dept Phys & Astron, POB 6315, Morgantown, WV 26506 USA
[10] West Virginia Univ, Ctr Gravitat Waves & Cosmol, Chestnut Ridge Res Bldg, Morgantown, WV 26505 USA
[11] CSIRO Astron & Space Sci, Australia Telescope Natl Facil, POB 76, Epping, NSW 1710, Australia
[12] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC V6T 1Z1, Canada
[13] Auckland Univ Technol, Inst Radio Astron & Space Res, Private Bag 92006, Auckland 1142, New Zealand
[14] Argelander Insitut Astron, Hugel 71, D-53121 Bonn, Germany
[15] Univ Bielefeld, Fak Phys, Postfach 100131, D-33501 Bielefeld, Germany
基金
欧洲研究理事会; 英国科学技术设施理事会; 美国国家科学基金会;
关键词
gravitation; surveys; binaries: close; pulsars: individual: PSR J1757-1854; RELATIVISTIC CELESTIAL MECHANICS; GENERAL-RELATIVITY; DISCOVERY; GRAVITY; SYSTEMS; SEARCH; TESTS;
D O I
10.1093/mnrasl/sly003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of PSR J1757-1854, a 21.5-ms pulsar in a highly-eccentric, 4.4-h orbit with a neutron star (NS) companion. PSR J1757-1854 exhibits some of the most extreme relativistic parameters of any known pulsar, including the strongest relativistic effects due to gravitational-wave damping, with a merger time of 76 Myr. Following a 1.6-yr timing campaign, we have measured five post-Keplerian parameters, yielding the two component masses (m(p) = 1.3384(9) M-circle dot and m(c) = 1.3946(9) M-circle dot) plus three tests of general relativity, which the theory passes. The larger mass of the NS companion provides important clues regarding the binary formation of PSR J1757-1854. With simulations suggesting 3-sigma measurements of both the contribution of Lense-Thirring precession to the rate of change of the semimajor axis and the relativistic deformation of the orbit within similar to 7-9 yr, PSR J1757-1854 stands out as a unique laboratory for new tests of gravitational theories.
引用
收藏
页码:L57 / L61
页数:5
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