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Magnetic Fields in Young SNRs

  • John R. Dickel (a1) and Eric M. Jones (a2)

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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.

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References

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Magnetic Fields in Young SNRs

  • John R. Dickel (a1) and Eric M. Jones (a2)

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