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Galactic HI Mapping and Optical–IR Studies

Published online by Cambridge University Press:  05 March 2013

R. D. Davies*
Affiliation:
Nuffield Radio Astronomy Laboratories, University of Manchester, Jodrell Bank, Macclesfield, Cheshire, SK11 9DL, UK. [email protected]
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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
Copyright
Copyright © Astronomical Society of Australia 1997

References

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