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Contents Page: Volume 14, Number 1

Galactic HI mapping and optical-IR studies.

R.D. Davies
University of Manchester, Nuffield Radio Astronomy Laboratories,
Jodrell Bank, Macclesfield, Cheshire, SK11 9DL, UK.


HI structure is seen at every scale down to the angular resolution limit of all survey telescopes. I present several examples of the structures at high Galactic latitudes with the 12 arcmin beam of the Lovell Telescope, the 2 arcmin resolution of the DRAO synthesis, as well as other indicators of finer scale structure in the interstellar medium (ISM).

Keywords: The Galaxy: structure-- Interstellar medium-- Instrumentation: miscellaneous

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