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Gravitational perturbations as a source of timing noise
Published online by Cambridge University Press: 12 April 2016
Abstract
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