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An AU-Aperture Lens to Resolve the Vela Pulsar’s Radio Emission Region
Published online by Cambridge University Press: 12 April 2016
Abstract
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We use radio-wave scattering in the Vela supernova remnant, surrounding the Vela pulsar, as an AU-scale lens to study the Vela pulsar’s emission region.
- Type
- Part 6 Winds and the ISM
- Information
- International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 459 - 461
- Copyright
- Copyright © Astronomical Society of the Pacific 1996
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