Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-26T22:18:39.100Z Has data issue: false hasContentIssue false

A UKST Hα Survey of the Galactic Plane

Published online by Cambridge University Press:  05 March 2013

Q. A. Parker
Affiliation:
Anglo-Australian Observatory, Coonabarabran, NSW 2357, Australia. , [email protected]
Q. S. Phillipps
Affiliation:
University of Bristol, Tyndal Avenue, Bristol, UK.
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We describe a major Anglo-Australian project to undertake a UKST Ha survey of the Southern Galactic plane, Magellanic clouds and selected regions. The survey will use a new 12 × 12 inch monolithic Hα interference filter of high specification and Tech Pan film which offers significant advantages over other emulsions due to its peak sensitivity at Ha and its extremely fine grain, high resolution, exceptional DQE, excellent imaging and low noise. A survey of unprecedented area coverage, depth and resolution should result, superior to any previous optical survey of ionised gas in the galaxy. It is certain to lead to exciting new discoveries and new avenues of research.

Type
Hi in the Local Universe
Copyright
Copyright © Astronomical Society of Australia 1997

References

Parker, Q. A., Phillipps, S., & Morgan, D. H. 1995, IAU Colloq. No. 148, ASP Conf. Ser. 84, ed. J. M. Chapman et al. (San Francisco: ASP), 129 Google Scholar
Davies, R. S., Elliot, K. H., & Meaburn, J. 1976, Mem. RAS, 81, 89 Google Scholar