Article contents
Geodetic Precession in PSR B1534+12
Published online by Cambridge University Press: 12 April 2016
Abstract
We present Arecibo observations of PSR B1534+12 which confirm previous suggestions that the pulse profile is evolving secularly. This effect is similar to that seen in PSR B1913+16, and is almost certainly due to general relativistic precession of the pulsar’s spin axis.
- Type
- Part 2. Timing, General Relativity and Astrometry
- Information
- International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 121 - 124
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
References
- 5
- Cited by