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

Recent radio and polarization observations

of dwarf irregulars

Krzysztof T. Chyzy, Sven Kohle, Rainer Beck,

Uli Klein, and Marek Urbanik

 [Fig. 1]
Fig. 1. The total power contours of NGC 4449 at 8.4 GHz with superimposed B-vectors of polarized intensity, overlaid upon the galaxy's Halpha image. A natural weighting and convolution to a beam of 15" was applied to the radio data, the total power map was also combined with a single dish one by Klein et al. (1996)
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First version: 10thAugust,1998
Last update: 29thSeptember,1998
Jochen M. Braun   &   Tom Richtler
 (E-Mail: jbraun|richtler@astro.uni-bonn.de)