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Galactic HI Mapping and Optical–IR Studies
Published online by Cambridge University Press: 05 March 2013
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 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
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- Copyright © Astronomical Society of Australia 1997