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Title:
Pulsar timing. I - Observations from 1970 to 1978
Authors:
Helfand, D. J.; Taylor, J. H.; Backus, P. R.; Cordes, J. M.
Affiliation:
AA(Massachusetts, University, Amherst, Mass; Columbia University, New York, N.Y.), AB(Massachusetts, University, Amherst, Mass.), AC(Massachusetts, University, Amherst, Mass.), AD(Massachusetts, University, Amherst, Mass.)
Publication:
Astrophysical Journal, Part 1, vol. 237, Apr. 1, 1980, p. 206-215. (ApJ Homepage)
Publication Date:
04/1980
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
Astrometry, Pulsars, Stellar Rotation, Time Measurement, Neutron Stars, Noise Measurement, Stellar Magnetic Fields, Stellar Models
DOI:
10.1086/157860
Bibliographic Code:
1980ApJ...237..206H

Abstract

The results of a series of pulsar timing programs spanning eight years were presented. The data have yielded accurate periods, period derivatives, and positions for three-dozen sources. Proper motions for three pulsars have been determined, useful upper limits have been derived for most of the remaining objects, and limits have been placed on possible dispersion measure changes. The timing noise phenomenon, first seen in the Crab pulsar, has been established as a general characteristic of pulsar rotation rates.

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