Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-27T00:25:20.479Z Has data issue: false hasContentIssue false
  • English
  • Français

Binary Pulsars

Published online by Cambridge University Press:  14 August 2015

Joseph H. Taylor
Joseph H. Taylor*
Affiliation:
University of Massachusetts, Amherst

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

There are now three radio frequency pulsars known to be in binary systems: PSRs 1913+16, 0820+02, and 0655+64. The first of these, discovered in 1974, moves in a tight, highly eccentric orbit with a period of approximately 7h 45m. Its companion has not yet been identified with certainty, but must be a compact object of mass comparable to that of the pulsar. PSRs 0820+02 and 0655+64, recognized as binaries during the past fifteen months, have nearly circular orbits with periods of over three years and about one day, respectively. All three objects are of great interest for the opportunity they provide to measure the masses of neutron stars. In addition, the first has proven to be a useful probe of gravitational theories, and the study of all of them should yield important information concerning the evolution of binary systems and the formation of neutron stars.

Type
VIII. Neutron Stars in Binary Systems
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 361 - 369
Copyright
Copyright © Reidel 1981 

References

Blandford, R.D. and De Campli, W.M.: 1981, this volume.Google Scholar
Blandford, R.D. and Teukolsky, S.A.: 1976, Astrophys. J. 205, p. 580.Google Scholar
Damashek, M., Backus, P.R. and Taylor, J.H.: 1980, in preparation.Google Scholar
Damashek, M., Taylor, J.H. and Hulse, R.A.: 1978, Astrophys. J. (Letters) 255, p. L31.CrossRefGoogle Scholar
Epstein, R.: 1977, Astrophys. J. 216, p. 92.Google Scholar
Hari-Dass, N.D. and Radhakrishnan, V.: 1975, Astrophys. Letters 16, p. 135.Google Scholar
Hulse, R.A. and Taylor, J.H.: 1975, Astrophys. J. (Letters) 195, p.L51.Google Scholar
Manchester, R.N., Lyne, A.G., Taylor, J.H., Durdin, J.M., Large, M.I. and Little, A.G.: 1978, Mon. Not. Roy. Astron. Soc. 185, p. 409.Google Scholar
Manchester, R.N., Newton, L.M., Cooke, D.J. and Lyne, A.G.: 1980, Astrophys. J. (Letters) 236, p. L25.Google Scholar
McCulloch, P.M., Taylor, J.H. and Weisberg, J.M.: 1979, Astrophys. J. (Letters) 227, p. L133.Google Scholar
Peters, P.C. and Matthews, J.: 1963, Phys. Rev. 131, p. 435.Google Scholar
Taylor, J.H., Fowler, L.A. and McCulloch, P.M.: 1979, Nature 227, p. 437.Google Scholar
Taylor, J.H., Hulse, R.A., Fowler, L.A., Gullahorn, G.E. and Rankin, J.M.: 1976, Astrophys. J. (Letters) 206, p. L53.Google Scholar