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Polarization in the Magellanic Clouds

Published online by Cambridge University Press:  25 April 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:
Australia Telescope National Facility, CSIRO, P.O. Box 76, Epping, NSW 2121
S. Wayte
Affiliation:
Mount Stromlo and Siding Spring Observatories
J. I. Harnett
Affiliation:
University of Sydney
U. Klein
Affiliation:
Max-Planck-lnstitut für Radioastronomie University of Bonn
R. Wielebinski
Affiliation:
Mount Stromlo and Siding Spring Observatories
U. R. Buczilowski
Affiliation:
Mount Stromlo and Siding Spring Observatories
E. Bajaja
Affiliation:
Mount Stromlo and Siding Spring Observatories
D. Malin
Affiliation:
Anglo-Australian Observatory
J. D. Murray
Affiliation:
Australia Telescope National Facility, CSIRO, P.O. Box 76, Epping, NSW 2121
A. J. Hunt
Affiliation:
Australia Telescope National Facility, CSIRO, P.O. Box 76, Epping, NSW 2121
R. Wark
Affiliation:
Australia Telescope National Facility, CSIRO, P.O. Box 76, Epping, NSW 2121
L. Sciacca
Affiliation:
Australia Telescope National Facility, CSIRO, P.O. Box 76, Epping, NSW 2121
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Abstract

We present preliminary results from a number of deep radio polarization surveys being made of the Magellanic Clouds at 2.3 GHz, 4.75 GHz and 8.55 GHz. Extended and linearly polarized radio emission has been found at 2.3 and 4.75 GHz from both the Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC). However, as the analysis of these data is not yet complete we present only some of the 4.75 GHz results at this time.

Type
Extragalactic
Information
Publications of the Astronomical Society of Australia , Volume 8 , Issue 4 , 1990 , pp. 339 - 342
Copyright
Copyright © Astronomical Society of Australia 1990

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