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

© Copyright Astronomical Society of Australia 1997