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Pulsar (and X-Star) Emission from the Magnetosphere of a Collapsed Star
Published online by Cambridge University Press: 07 February 2017
Abstract
We propose nonthermal plasma mechanisms to account for the most evident physical characteristics of pulsar emission, including the production of X- and γ-rays and the acceleration of high-energy particles. Special reference to the Crab Nebula pulsar (NP 0532) is made and an application of the same model to other non-thermal X-ray sources is suggested.
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- Copyright © Reidel 1971