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Polarization in the Magellanic Clouds

Published online by Cambridge University Press:  19 July 2016

R.F. Haynes ,
S. Wayte ,
J.I. Harnett ,
U. Klein ,
R. Wielebinski ,
U.R. Buczilowski ,
E. Bajaja ,
D. Malin ,
J.D. Murray  and
A.J. Hunt
...Show all authors
R.F. Haynes
Affiliation:
1. Australia Telescope National Facility#
S. Wayte
Affiliation:
4. Mount Stromlo and Siding Spring Observatories
J.I. Harnett
Affiliation:
5. University of Sydney
U. Klein
Affiliation:
2. Max-Planck-Institut für Radioastronomie 3. University of Bonn
R. Wielebinski
Affiliation:
2. Max-Planck-Institut für Radioastronomie
U.R. Buczilowski
Affiliation:
2. Max-Planck-Institut für Radioastronomie
E. Bajaja
Affiliation:
2. Max-Planck-Institut für Radioastronomie
D. Malin
Affiliation:
6. Anglo-Australian Observatory
J.D. Murray
Affiliation:
1. Australia Telescope National Facility#
A.J. Hunt
Affiliation:
1. Australia Telescope National Facility#
R. Wark
Affiliation:
1. Australia Telescope National Facility#
L. Sciacca
Affiliation:
1. Australia Telescope National Facility#

Abstract

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We present new results from a number of deep radio polarization surveys of the Magellanic Clouds at 2.3 GHz, 4.75 GHz and 8.55 GHz. Extended linearly polarized radio emission has been found at 2.3 and 4.75 GHz from both galaxies.

Type
5. The Polarization, Magnetic Field and Velocity Structure of External Spiral Galaxies
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 205 - 209
Copyright
Copyright © Kluwer 1990 

References

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