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Magnetic Fields in Young SNRs

Published online by Cambridge University Press:  19 July 2016

John R. Dickel  and
Eric M. Jones
John R. Dickel
Affiliation:
University of Illinois & Los Alamos National Laboratory
Eric M. Jones
Affiliation:
Los Alamos National Laboratory

Extract

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There are two very important properties of the magnetic fields in supernova remnants which we wish to emphasize: 1) The net radial orientation of the magnetic vectors throughout the shell and 2) an apparent gradual increase in the fractional polarization with evolutionary age.

Type
3. Magnetic Fields in and around Supernova Remnants
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 81 - 82
Copyright
Copyright © Kluwer 1990 

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