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Pulsar PRS 0656 + 14 - Period and spindownObservations from various sources are used to explain the larger-than-expected period noted for pulsar 0656 + 14 on July 7, 1984 (Ashworth and Lyne, 1981). No indication of orbital motion was found, and most of the observations are consistent with a simple secular spindown. The derived period derivative of (54.3 + or - 1.3) x 10 to the -15th at epoch 2444300 is far greater than the previously reported value.
Document ID
19860063752
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Domingue, D.
(Vermont Univ. Burlington, VT, United States)
Rankin, J. M.
(Vermont, University Burlington, United States)
Weisberg, J. M.
(Carleton College Northfield, MN, United States)
Backus, P. R.
(NASA Ames Research Center Mountain View, CA, United States)
Date Acquired
August 12, 2013
Publication Date
June 1, 1986
Publication Information
Publication: Astronomy and Astrophysics
Volume: 161
Issue: 2, Ju
ISSN: 0004-6361
Subject Category
Astrophysics
Accession Number
86A48490
Distribution Limits
Public
Copyright
Other

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