No CrossRef data available.
Article contents
The Potential for Astronomy in the Infrared*
Published online by Cambridge University Press: 02 August 2016
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.
Infrared Interferometry promises to be a useful astrometric technique. Preliminary measurements of the star α Orionis made with a heterodyne interferometer exhibit phase coherence over a period of at least 1000 seconds. The measurements were equivalent to a positional determination of 60 second accuracy every 5 seconds of integration.
- Type
- The Scientific Programme
- Information
- International Astronomical Union Colloquium , Volume 50: High Angular Resolution Stellar Interferometry , January 1979 , pp. 20-1 - 20-12
- Copyright
- Copyright © 1979
Footnotes
*
This work is supported in part by NASA Grant NGL 05-003-272 and NSF Grant AST 77-12256
References
1)
Tatarski, V.I., “Wave Propagation in a Turbulent Medium”, McGraw Hill, 1961.CrossRefGoogle Scholar
5)
Zhevakin, S.A. and Naumov, A.P., Radiotekhnika i Elecktronika, 12, 885, 1967 and 12, 1067, 1967.Google Scholar
6)
Townes, C.H., Sutton, E.C. and Storey, J.W.V., “Optical Telescopes of the Future,” Conference Proceedings, December 1977, Geneva 23: ESO c/o CERN, 1978.Google Scholar
7)
Hall, R.T., “A Catalog of 10 urn Celestial Objects”, Report SAMSO-TR-74-212, Space and Missile Systems Organization, Airforce Systems Command, Los Angeles, 1974.Google Scholar
8)“Apparent Places of Fundamental Stars”, Heidelberg: Astronomisches Rechen-Institut.Google Scholar
You have
Access