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Gravitational perturbations as a source of timing noise

Published online by Cambridge University Press:  12 April 2016

A. E. Rodin
A. E. Rodin*
Affiliation:
PRAO ASC LPI, Pushchino, Moscow region, 142292, Russia

Abstract

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In assumption that pulsar gravitationally interacts with its surroundings the relationships between the pulsar rotational and orbital parameters are derived and the solutions for PSR B1620–26 and PSR B1822–09 are presented.

Type
Part 2. Timing, General Relativity and Astrometry
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 105 - 106
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

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