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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

Bruno Coppi  and
Attilio Ferrari
Bruno Coppi
Affiliation:
Massachusetts Institute of Technology, Cambridge, Mass., U.S.A.
Attilio Ferrari
Affiliation:
Laboratorio di Cosmo-geofisica del CNR and Istituto di Fisica dell'Università, Torino, Italy

Abstract

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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.

Type
Session 8
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 460 - 470
Copyright
Copyright © Reidel 1971 

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