Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-20T08:36:32.401Z Has data issue: false hasContentIssue false

Relationship Between Pulsar and Nebula

Published online by Cambridge University Press:  07 February 2017

L. Woltjer*
Affiliation:
Department of Astronomy, Columbia University, New York, N.Y., U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The magnetic field and the relativistic electrons in the Crab Nebula cannot have originated at the time of the supernova explosion. The energy density in the magnetic field is so large that it must have been generated using the energy supply in the pulsar. The energies of the electrons are so high, and their lifetimes correspondingly are so short, that they must have been accelerated, again using the pulsar energy. The efficiency of these processes must be high, but there is an adequate energy supply.

Type
Session 7
Copyright
Copyright © Reidel 1971 

References

Goldreich, P. and Julian, W. H.: 1969, Astrophys. J. 157, 869.CrossRefGoogle Scholar
Gunn, J. E. and Ostriker, J. P.: 1969, Astrophys. J. 157, 1395.Google Scholar