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Pulsar PSR 0656+14: period and spindownOn July 7, 1984 pulsar 0656+14 was found to exhibit a larger period than expected. Using observations from a number of sources, we have attempted to explain this discrepancy. No indications of orbital motion was found. The available evidence indicates that the star has a period derivative of 54 10(-15) s s-1 rather than 1.6 10(-15) s s-1 as previously reported.
Document ID
20040089133
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Domingue, D.
(University of Vermont Burlington 05405, United States)
Rankin, J. M.
Weisberg, J. M.
Backus, P. R.
Date Acquired
August 21, 2013
Publication Date
January 1, 1986
Publication Information
Publication: Astronomy and astrophysics
Volume: 161
ISSN: 0004-6361
Subject Category
Exobiology
Report/Patent Number
ISSN: 0004-6361
Distribution Limits
Public
Copyright
Other
Keywords
NASA Center ARC
NASA Discipline Exobiology
Astronomy/methods
Extraterrestrial Environment
Least-Squares Analysis

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