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A New Very High Angular Resolution Stellar Interferometer

Published online by Cambridge University Press:  25 April 2016

J . Davis  and
W . J . Tango
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Abstract

The Chatterton Astronomy Department of the University of Sydney is proposing the construction of a very high angular resolution stellar interferometer of major astronomical and international significance. Based on the prototype modern Michelson stellar interferometer which the Department has developed, the new instrument will be used in a wide range of astrophysical programmes. The siting, specification, design and costing of the instrument are outlined.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 6 , Issue 1 , 1985 , pp. 38 - 43
Copyright
Copyright © Astronomical Society of Australia 1985

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References

Davis, J., 1976, Proc. Astron. Soc. Aust., 3, 26.Google Scholar
Davis, J., 1979, in ‘High Angular Resolution Stellar Interferometry (I.A.U. Colloquium No. 50)’, (eds Davis, J. and Tango, W. J.), p. 1.1 (Chatterton Astronomy Department, University of Sydney).Google Scholar
Davis, J., 1984, in ‘Indirect Imaging’ (ed. J. A. Roberts), p. 125 (Cambridge University Press).Google Scholar
Davis, J., and Tango, W. J., 1985, Proc. Astron. Soc. Aust., 6, 34.Google Scholar
McAlister, H. A., 1979, in ‘High Angular Resolution Stellar Interferometry (I.A.U. Colloquium No. 50)’, (eds Davis, J. and Tango, W. J.), p. 3.1 (Chatterton Astronomy Department, University of Sydney).Google Scholar
Tango, W. J., 1979, in ‘High Angular Resolution Stellar Interferometry (I.A.U. Colloquium No. 50)’, (eds Davis, J. and Tango, W. J.)), p. 12.1 (Chatterton Astronomy Department, University of Sydney).Google Scholar
Tango, W. J., and Twiss, R. Q., 1980, Progress in Optics, XVII, 241.Google Scholar