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Twelve years of Glitches in the Vela Pulsar
Published online by Cambridge University Press: 12 April 2016
Extract
The Vela pulsar (PSR B0833–45) has been observed from Hartebeesthoek RAO since 1984, as part of an ongoing monitoring project. During this time, the pulsar has undergone five sudden and relatively large spin-ups (“glitches”). Good observational coverage was obtained for the four most recent of these events.
The post-glitch behaviour of (t) is modelled by:
- Type
- Part 2 Precision Measurements
- Information
- International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 103 - 104
- Copyright
- Copyright © Astronomical Society of the Pacific 1996