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Interpretation of Binary Pulsar Observations

Published online by Cambridge University Press:  14 August 2015

R. D. Blandford  and
W. M. DeCampli
R. D. Blandford
Affiliation:
California Institute of Technology
W. M. DeCampli
Affiliation:
California Institute of Technology

Abstract

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The nature, dynamics and evolution of the three known radio pulsar binaries are discussed. The system containing 1913+16 appears to comprise two ~1.4 M⊙ components, and to undergo orbital decay as predicted by general relativity. It is proposed that 1913+16 has a neutron star companion and that 0655+64 and 0820+02 have white dwarf companions which should be observable optically.

Type
VIII. Neutron Stars in Binary Systems
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 371 - 378
Copyright
Copyright © Reidel 1981 

References

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