Galactic H I mapping and optical-IR studies.
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).
- Publication:
-
Publications of the Astronomical Society of Australia
- Pub Date:
- April 1997
- DOI:
- 10.1071/AS97118
- Bibcode:
- 1997PASA...14..118D