Abstract
We describe 21-cm line observations of the Draco nebula region and present the results as channel maps. These observations have been performed with the Effelsberg 100-m telescope, the Westerbork Synthesis Radiotelescope, and the Very Large Array. The measurements reveal the full extent of the cloud as well as the detailed morphological and kinematical structure of several subareas. A list of continuum point sources found in the aperture synthesis maps is included.
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