Published 1981
| Published
Book Section - Chapter
Open
Interpretation of Binary Pulsar Observations
- Creators
-
Blandford, R. D.
- DeCampli, W. M.
- Others:
- Sieber, Wolfgang
- Wielebinski, R.
Chicago
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Abstract
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.
Additional Information
© 1981 by the IAU. We thank J. Condon, E. Feigelson, P. Goldreich, J. Kristian, P. Scheuer, J. Taylor and P. Young for discussions and permission to quote data before publication. This research was supported in part by NSF grant AST78-05484 and the Weizmann Foundation.Attached Files
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interpretation_of_binary_pulsar_observations.pdf
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Additional details
- Eprint ID
- 91665
- Resolver ID
- CaltechAUTHORS:20181211-074758932
- NSF
- AST 78-05484
- Weizmann Foundation
- Created
-
2018-12-11Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field
- Series Name
- IAU Symposium Proceedings Series
- Series Volume or Issue Number
- 95