Hostname: page-component-78c5997874-94fs2 Total loading time: 0 Render date: 2024-11-05T09:58:14.836Z Has data issue: false hasContentIssue false
  • English
  • Français

The Crab Pulsar as a Component of a Binary System

Published online by Cambridge University Press:  14 August 2015

A. I. Tsygan
A. I. Tsygan*
Affiliation:
A. F. Ioffe Physical Technical Institute, Academy of Sciences, Leningrad, U.S.S.R.

Abstract

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.

This note discusses the properties of the Crab pulsar assuming that it is moving in the gravitational field of the second component.

Type
Part 9 / Variable X-Ray Sources
Information
Symposium - International Astronomical Union , Volume 67: Variable Stars and Stellar Evolution , 1975 , pp. 499 - 500
Copyright
Copyright © Reidel 1975 

References

Boynton, P. E., Groth, E. J., Hutchinson, D. P., Nanos, G. P., Partridge, R. B. Jr. and Wilkinson, D. T.: 1972, Astrophys. J. 175, 217.Google Scholar
Conner, J. P., Evans, W. D. and Belian, R. D.: 1969, Astrophys. J. 157, L157.Google Scholar
Richards, D. W., Pettengill, G. H., Counselman, C.C. III, and Rankin, J. M.: 1970, Astrophys. J. 160, L1.CrossRefGoogle Scholar
Ruderman, M.: 1972, Ann. Rev. Astron. Astrophys. 10, 427.CrossRefGoogle Scholar
Shklovsky, I. S.: 1968, Supernovae, Wiley-Interscience, London, chap. III.Google Scholar