Hostname: page-component-7479d7b7d-wxhwt Total loading time: 0 Render date: 2024-07-11T08:29:11.884Z Has data issue: false hasContentIssue false
  • English
  • Français

Infrared Spectroscopy in Australia

Published online by Cambridge University Press:  25 April 2016

Terry Jay Jones
Terry Jay Jones*
Affiliation:
Mt Stromlo and Siding Spring Observatory, A.N.U.
Get access Rights & Permissions [Opens in a new window]

Extract

Infrared spectroscopy is a relatively new field in astronomy. When the study of celestial sources at wavelengths longer than 1 μm underwent a major spurt of growth in the mid-sixties, it was natural for astronomers to concentrate on broad band measurements. As detectors and instrumentation have steadily improved and the broad band characteristics of stellar sources in the IR have become better known, there has been a natural trend to higher spectral resolution. To date there has been sufficient work in IR spectroscopy to warrant several reviews on the subject. Although Australia has been late in entering this exciting and expanding field, the quality of work has more than made up for the delay. In this review I will briefly describe several projects involving IR spectra performed in Australia. Special emphasis will be placed on those experiments that cannot be done by any means other than IR spectroscopy. Also presented is a description of Australia’s next generation of spectroscopic instrumentation for the IR.

Type
Invited Papers
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 2 , 1981 , pp. 152 - 155
Copyright
Copyright © Astronomical Society of Australia 1981

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Aitken, D. K. Private communication (1981).Google Scholar
Aitken, D. K., and Roche, P. F. Submitted Mon. Not. Astron. Soc. (1981).Google Scholar
Aitken, D. K., Roche, P. F., Spenser, P. M, and Jones, B. Astron. Astrophys., 76, 60 (1979a).Google Scholar
Aitken, D. K., Roche, P. F., Spenser, P. M., and Jones, B. Astrophys. J., 233, 925 (1979b).Google Scholar
Aitken, D. K., Roche, P. F., Spenser, P. M., and Jones, B. Mon. Not. Astron. Soc., 195, in press (1981).Google Scholar
Allen, D. A. Nature, 284, 323 (1980).Google Scholar
Allen, D. A. Private communication (1981).Google Scholar
Allen, D. A., Barton, J. R., Gillingham, P. R., and Carswell, R. F. Submitted Mon. Not. Astron. Soc. (1981).Google Scholar
Barton, J. R., Phillips, B. A., and Allen, D. A. Mon. Not. Astron. Soc., 187, 813 (1979).Google Scholar
Blades, J. C., and Whittet, D. C. B. Mon. Not. Astron. Soc., 191, 701 (1980).CrossRefGoogle Scholar
Hillier, J. Private communication (1981).Google Scholar
Jones, T. J., Hyland, A. R., Caswell, J. L., and Gatley, I. Astrophys. J., submitted (1981).Google Scholar
McGregor, P., and Hyland, A. R. Submitted Astrophys. J. (1981a).Google Scholar
McGregor, P. Submitted Astrophys. J. (1981b).Google Scholar
Whiteoak, J. B., and Gardner, F. F. Private communication (1981).Google Scholar
Whittet, D. C. B., and Blades, J. C. Mon. Not. Astron. Soc., 191, 309 (1980).Google Scholar
Williams, P. M., and Allen, D. A. Observ., 100, 202 (1980).Google Scholar