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Pulsar Position, Proper Motion, and Parallax via VLBI
Published online by Cambridge University Press: 12 April 2016
Abstract
I briefly review the means by which VLBI observations can determine the position, proper motion, and parallax of a pulsar, and consider a small subset of the applications of such results.
- Type
- Part 2. Timing, General Relativity and Astrometry
- Information
- International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 135 - 138
- Copyright
- Copyright © Astronomical Society of the Pacific 2000