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Radio continuum emission from the Magellanic Clouds

Published online by Cambridge University Press:  19 July 2016

U. Klein ,
R.F. Haynes ,
R. Wielebinski ,
S.R. Wayte ,
J.I. Harnett ,
E. Bajaja ,
J.D. Murray ,
A.J. Hunt ,
R. Wark  and
L. Sciacca
...Show all authors
U. Klein
Affiliation:
Max-Planck-Institut für Radioastronomie
R.F. Haynes
Affiliation:
Australia Telescope National Facility
R. Wielebinski
Affiliation:
Max-Planck-Institut für Radioastronomie
S.R. Wayte
Affiliation:
Mount Stromlo and Siding Spring Observatories
J.I. Harnett
Affiliation:
University of Sydney
E. Bajaja
Affiliation:
Instituto Argentino de Radioastronomia
J.D. Murray
Affiliation:
Australia Telescope National Facility
A.J. Hunt
Affiliation:
Australia Telescope National Facility
R. Wark
Affiliation:
Australia Telescope National Facility
L. Sciacca
Affiliation:
Australia Telescope National Facility
U. R. Buczilowski
Affiliation:
Max-Planck-Institut für Radioastronomie

Abstract

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New radio continuum surveys of the Large and the Small Magellanic Cloud have been completed recently at four frequencies, using the Parkes 64-m telescope. Here we shall discuss briefly the overall radio morphology of the Clouds at different frequencies and discuss the detected linear polarization. A preliminary integrated radio continuum spectrum of the Large Magellanic Cloud is also presented. Various aspects of future studies will be outlined.

Type
Large-Scale Structure and Kinematics
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 31 - 35
Copyright
Copyright © Kluwer 1991 

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