Parametric matching of the dispersion measure in observed pulsar time intervals

It is shown that there is a parametric connection between the dispersion measure and the observed pulsar rotation period. The conditions for them to agree are determined, and theoretical relations and numerical estimates are obtained.

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Bibliographic Details
Published in:Measurement techniques 2010-09, Vol.53 (5), p.525-532
Main Author: Avramenko, A. E.
Format: Article
Language:English
Subjects:
Analysis
Analytical Chemistry
Astronomy
Characterization and Evaluation of Materials
Dispersions
Estimates
Intervals
Joints
Matching
Measurement Science and Instrumentation
Measurement techniques
Measures of variability
Physical Chemistry
Physics
Physics and Astronomy
Pulsars
Radio telescopes
Scientific imaging
Studies
Telescopes
Time and Frequency Measurements
Trends
Citations: Items that this one cites
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Description
Summary:It is shown that there is a parametric connection between the dispersion measure and the observed pulsar rotation period. The conditions for them to agree are determined, and theoretical relations and numerical estimates are obtained.
ISSN:0543-1972
1573-8906
DOI:10.1007/s11018-010-9537-3