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The Parallax And Proper Motion Program Of The Shanghai Observatory 1.56-M Astrometric Reflector
Published online by Cambridge University Press: 03 August 2017
Abstract
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The main properties of the 1.56-m astrometric reflector of Shanghai Observatory are described. Some principles of selecting program stars are presented. The experimental program that has been performed with the Zô-sè 40-cm refractor since 1980 is outlined. Accuracies which are expected to be obtained for new program parallaxes are discussed.
- Type
- Part II: Current Research
- Information
- Copyright
- Copyright © Kluwer 1988
References
Moffett, T. J., Barnes, T. G., and Evans, D. S., 1985, Calibration of Fundamental Stellar Quantities, edited by Hayes, D. S. et al. (Reidel, Dordrecht), p. 365.Google Scholar