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Studying Pulsar Emission Regions Using Interstellar Scattering
Published online by Cambridge University Press: 12 April 2016
Abstract
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Radio-wave scattering in the interstellar plasma provides the means to circumvent the diffraction limit for earth-based instruments, and to image the emission regions of pulsars. For the past 25 years, observers have sought to exploit this fact to learn how pulsars shine. I review the techniques developed, and summarize measurements of size of emission regions of pulsars to date.
- Type
- Chapter Two Pulsars: Their Scattering and Intrinsic Properties
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- Copyright
- Copyright © Kluwer 2001
References
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