Proceedings of the Workshop
"The Magellanic Clouds and Other Dwarf Galaxies"
of the Bonn/Bochum-Graduiertenkolleg

The ATCA Radio-continuum Investigation of the Magellanic Clouds

Miroslav D. Filipovic and Lister Staveley-Smith

 [Fig. 1]
Fig. 1. The mosaic radio-continuum image of the SMC at 2.3 GHz (λ=13 cm). The image is corrected for the short spacing missing flux by adding/combining Parkes data from the same frequency. The observed beam size is 45" and is shown in the lower left corner. Over seven hundred sources were found in this survey
[Fig. 2]
Fig. 2. The ``snap-shot'' images of the SMC SNR N 76 at (a) λ=6 cm and (b) λ=3 cm. The observed beam size is 30" at λ=6 cm and 15" at λ=3 cm. The beams are shown in the lower right corner
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First version: 13thJuly,1998
Last update: 27thSeptember,1998
Jochen M. Braun   &   Tom Richtler
 (E-Mail: jbraun|richtler@astro.uni-bonn.de)