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SNR Polarization and the Direction of the Magnetic Field

Published online by Cambridge University Press:  12 April 2016

D.K. Milne
D.K. Milne*
Affiliation:
Division of Radiophysics, CSIRO, PO Box 76 Epping, NSW 2121, Australia

Abstract

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At the CSIRO Division of Radiophysics we are currently engaged in a program to map polarization in SNRs at 8.4 GHz. These results are compared with earlier Parkes 5 GHz maps to deduce the direction of magnetic field, Faraday rotation and depolarization.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 351 - 354
Copyright
Copyright © Cambridge University Press 1988

References

Caswell, J.L. (1977). Proc. Astron. Soc. Aust. 3, 130.Google Scholar
Caswell, J.L., and Lerche, I. (1979). Mon. Not. R. Astron. Soc. 187, 201.Google Scholar
Milne, D.K. (1979). Aust. J. Phys. 32, 83.Google Scholar
Milne, D.K. (1987). “An atlas of SNR magnetic fields”, Aust. J. Phys. (in press).Google Scholar
Milne, D.K., and Dickel, J.R. (1975). Aust. J. Phys, 28, 209 CrossRefGoogle Scholar
Milne, D.K., Roger, R.S., Kesteven, M.J., Haynes, R.F., Wellington, K.J., and Stewart, R.T. (1986). Mon. Not. R. Astron. Soc. 223, 487 CrossRefGoogle Scholar
Milne, D.K., Roger, R.S., Kesteven, M.J., Haynes, R.F., and Wellington, K.J. (1987) (in preparation).Google Scholar
Roger, R.S., Milne, D.K., Caswell, J.L., and Little, A.G. (1986). Mon. Not. R. Astron. Soc. 219, 8.Google Scholar