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The Crab Pulsar as a Component of a Binary System

Published online by Cambridge University Press:  14 August 2015

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

Abstract

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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
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