Next Section: Introduction
Galactic HI mapping and optical-IR studies.
R.D. Davies
University of Manchester, Nuffield Radio Astronomy Laboratories,
Jodrell Bank, Macclesfield, Cheshire, SK11 9DL, UK.
email: rdd@jb.man.ac.uk
Abstract:
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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