Galactic HI mapping and optical-IR studies.
RD Davies
Publications of the Astronomical Society of Australia
14(1) 118 - 118
Published: 1997
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).https://doi.org/10.1071/AS97118
© ASA 1997