Hostname: page-component-5c6d5d7d68-sv6ng Total loading time: 0 Render date: 2024-08-26T10:12:19.404Z Has data issue: false hasContentIssue false
  • English
  • Français

The Parallax And Proper Motion Program Of The Shanghai Observatory 1.56-M Astrometric Reflector

Published online by Cambridge University Press:  03 August 2017

Wang Jia-ji
Wang Jia-ji*
Affiliation:
Shanghai Observatory Academia Sinica, Shanghai, People's Republic of China

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.

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
Symposium - International Astronomical Union , Volume 133: Mapping the Sky: Past Heritage and Future Directions , 1988 , pp. 479 - 482
Copyright
Copyright © Kluwer 1988 

References

Chiu, L.-T. G., 1977, Astron. J., 82, 842.Google Scholar
Eichhorn, H., and Jefferys, W. H., 1971, Publ. Leander McCormick Obs., 16, 267.Google Scholar
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
Monet, D. G., and Dahn, C. C., 1983, Astron. J., 88, 1489.Google Scholar
Murray, C. A., and Corben, P. M., 1979, Mon. Not. Roy. astr. Soc., 187, 723.Google Scholar
Upgren, A. R., 1982, Trans. IAU, 18B, 197.Google Scholar
Wang, J.-j., 1985, Annals of Shanghai Observatory Academia Sinica, 7, 26.Google Scholar