Search Swinburne Research Bank
Home List of Titles Self-consistency of relativistic observables with general relativity in the white dwarf-neutron star binary PSR J1141-6545
Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.3/1175
|Download PDF (Published version) (Adobe Acrobat PDF, 84 KB)|
- Self-consistency of relativistic observables with general relativity in the white dwarf-neutron star binary PSR J1141-6545
- Bailes, Matthew; Ord, Stephen M.; Knight, Haydon S.; Hotan, Aidan W.
- Here we report timing measurements of the relativistic binary PSR J1141-6545 that constrain the component masses and demonstrate that the orbital period derivative Pb=(-4+/-1)×10-13 is consistent with gravitational wave emission as described by the general theory of relativity. The mass of the neutron star and its companion are 1.30+/-0.02 and 0.986+/-0.02 Msolar, respectively, suggesting a white dwarf companion and extending the range of systems for which general relativity provides a correct description. On evolutionary grounds, the progenitor mass of PSR J1141-6545 should be near the minimum for neutron star production. Its mass is 2 standard deviations below the mean of the other neutron stars, suggesting a relationship between progenitor and remnant masses.
- Publication type
- Journal article
- Research centre
- Swinburne University of Technology. School of Biophysical Science and Electrical Engineering. Centre for Astrophysics and Supercomputing
- Astrophysical Journal Letters, Vol. 595, no. 1 (Sep 2003), pp. L49-L52
- Publication year
- Binaries: close; Gravitational waves; Neutron stars; Pulsars: general; Pulsars: individual (PSR J1141-6545); Relativity
- University of Chicago Press
- Publisher URL
- Copyright © 2003 The American Astronomical Society. Reproduced in accordance with the copyright policy of the publisher.
- Full text
- Peer reviewed