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ATCA Radio Polarization Observations of NGC 1566 and NGC 1672

Published online by Cambridge University Press:  19 July 2016

R. Beck ,
M. Ehle ,
R. F. Haynes  and
J. I. Harnett
R. Beck
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, FRG
M. Ehle
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, FRG
R. F. Haynes
Affiliation:
ATNF, Epping, Australia
J. I. Harnett
Affiliation:
Sydney University, Sydney, Australia

Abstract

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NGC 1566 and NGC 1672 have successfully been observed in radio continuum at 6 cm (26″ HPBW) with the Australia Telescope Compact Array (ATCA) using a 375-m array. We have detected for the first time with this telescope linearly polarized radio emission from two southern hemisphere spiral galaxies, NGC 1566 and NGC 1672.

Type
Imaging Results: Radio and Millimeter Waves
Information
Symposium - International Astronomical Union , Volume 158: Very High Angular Resolution Imaging , 1994 , pp. 358 - 360
Copyright
Copyright © Kluwer 1994 

References

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