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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

Davis, R. J., Diamond, R. J., & Goss, W. M. 1996, MNRAS, in pressGoogle Scholar
Hartmann, D., & Burton, W. B. 1996, An Atlas of Galactic Neutral Hydrogen Emission (Cambridge University Press), in pressGoogle Scholar
Heiles, C., Habing, H. J. 1974, ApJ SuppL, 14, 1 Google Scholar
Malawi, A., & Davis, R. D. 1996, in preparationGoogle Scholar
Shaw, C. R., Bates, B., Kemp, S. N., Keenan, F. F., Davies, R. D., & Roger, R. S., 1996, ApJ, in pressGoogle Scholar
Stark, A. A., et al. 1992, ApJ Suppl., 79, 77 Google Scholar
Trapero, J., Beckman, J. E., Serra-Rickart, M., Davies, R. D., Watson, R. A., & Garcia Lopez, R. J. 1995, ApJ, 445, 231 Google Scholar
Weaver, H. F., & Williams, D. R. 1973, ApJ Suppl., 8, 1 Google Scholar
Willacy, K., Pedlar, A., & Berry, D. 1993, MNRAS, 261, 165 Google Scholar