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Galactic HI Mapping and Optical–IR Studies

Published online by Cambridge University Press:  05 March 2013

R. D. Davies
R. D. Davies*
Affiliation:
Nuffield Radio Astronomy Laboratories, University of Manchester, Jodrell Bank, Macclesfield, Cheshire, SK11 9DL, UK. rdd@jb.man.ac.uk
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Abstract

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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 Loveli Telescope, the 2 arcmin resolution of the DRAO synthesis, as well as other indicators of finer scale structure in the interstellar medium (ISM).

Type
Hi in the Local Universe
Information
Publications of the Astronomical Society of Australia , Volume 14 , Issue 1 , 1997 , pp. 118 - 119
Copyright
Copyright © Astronomical Society of Australia 1997

References

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