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Radio Polarization and Magnetic Fields in Six Supernova Remnants

Published online by Cambridge University Press:  25 April 2016

D. K. Milne ,
J. L. Caswell ,
M. J. Kesteven ,
R. F. Haynes  and
R. S. Roger
D. K. Milne
Affiliation:
Australia Telescope National Facility, CSIRO, 1
J. L. Caswell
Affiliation:
Australia Telescope National Facility, CSIRO, 1
M. J. Kesteven
Affiliation:
Australia Telescope National Facility, CSIRO, 1
R. F. Haynes
Affiliation:
Australia Telescope National Facility, CSIRO, 1
R. S. Roger
Affiliation:
Dominion Radio Astronomical Observatory, Penticton BC, Canada
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Abstract

8.4 GHz linear polarization maps, obtained with the Parkes radio telescope, are presented for six southern supernova remnants. These results are compared with published and unpublished polarization maps at 5 GHz to derive the magnetic field direction and Faraday rotation measure distribution.

These results are part of a program to map the magnetic fields in galactic supernova remnants and complement our program to obtain high-resolution maps of galactic SNRs using the Molonglo Observatory Synthesis Telescope; five new Molonglo maps are presented here.

Type
Miscellaneous Radio Astronomy
Information
Publications of the Astronomical Society of Australia , Volume 8 , Issue 2 , 1989 , pp. 187 - 194
Copyright
Copyright © Astronomical Society of Australia 1989

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