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Single Pulse Polarimetry of the Vela Pulsar
Published online by Cambridge University Press: 12 April 2016
Abstract
Multi-frequency, single-pulse polarimetric observations of the Vela pulsar have been made using the VLA. These high time resolution measurements allow us to probe the geometry, and the time dependent characteristics of the radio emission region. Evidence for multiple emission components with differing spectral indices is found.
- Type
- Part 3. Studies of Radio Emission
- Information
- International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 257 - 260
- Copyright
- Copyright © Astronomical Society of the Pacific 2000