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Long Baseline Optical Interferometry

Published online by Cambridge University Press:  14 August 2015

S.T. Ridgway
S.T. Ridgway*
Affiliation:
Kitt Peak National Observatory, National Optical Astronomy Observatories, Box 26732, Tucson AZ 85726-6732, U.S.A.

Extract

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During the last three years significant results have been obtained from several operational, long baseline optical interferometers. Precision stellar angular diameters (accuracy of order 2% and better) have been reported in the infrared (DiBenedetto and Rabbia, 1987) and in the visible (Davis and Tango, 1986). Astrometric precision of order 20 milliarcsec has been demonstrated over large angles (Shao et al, in press). Spectro-spatial resolution of the disk of a Be star in the hydrogen emission line (Thom et al., 1986) suggests spectacular imaging science to come with many-telescope coherent and phased optical arrays.

Type
Joint Commission Meeting
Information
Highlights of Astronomy , Volume 8: Highlights of Astronomy. As presented at the XXth General Assembly of the IAU, 1988 , 1989 , pp. 559 - 560
Copyright
Copyright © Kluwer 1989

References

DiBenedetto, G.P. and Rabbia, Y., 1987, Astron. Astrophys.Google Scholar
Davis, J. and Tango, W.J., 1986, Nature 323 234–235.Google Scholar
Shao, M. et al. Astron. Astrophys. (in press).Google Scholar
Thom, C. et al. Astron. Astrophys. 165, L13–15.Google Scholar