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Evidence for Free Precession in the Pulsar B1642–03
Published online by Cambridge University Press: 12 April 2016
Abstract
The phase residuals of PSR B1642-03 obtained during a 30-yr interval since 1969 to 1999 are discussed. Interpretation of observed cyclical residual changes in terms of free precession gives a wooble angle of 0.3 - 0.7 degrees.
- Type
- Part 2. Timing, General Relativity and Astrometry
- Information
- International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 99 - 100
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
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