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Optical Determination In The Positions Of Radio Stars

Published online by Cambridge University Press:  03 August 2017

Xu Tong-qi ,
Lu Pei-zhen ,
Chu Zong-yuan  and
Wang Shu-he
Xu Tong-qi
Affiliation:
Shanghai Observatory Academia Sinica, Shanghai, People's Republic of China
Lu Pei-zhen
Affiliation:
Shanghai Observatory Academia Sinica, Shanghai, People's Republic of China
Chu Zong-yuan
Affiliation:
Shanghai Observatory Academia Sinica, Shanghai, People's Republic of China
Wang Shu-he
Affiliation:
Shanghai Observatory Academia Sinica, Shanghai, People's Republic of China

Abstract

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Optical positions of 16 radio stars have been derived from 40 cm astrograph at Zô-Sè. The reference catalogues are AGK3 and SAO, the average mean square error of single observation is 0″.058 in the right ascension and 0″.053 in declination. The magnitude difference has no significant effect on the observations.

Type
Part II: Current Research
Information
Symposium - International Astronomical Union , Volume 133: Mapping the Sky: Past Heritage and Future Directions , 1988 , pp. 497 - 500
Copyright
Copyright © Kluwer 1988 

References

Lu, P.-z., 1982, Annals of Shanghai Observatory, Academia Sinica, 4, 149.Google Scholar
Lu, P.-z., et al., 1985, Annals of Shanghai Observatory, Academia Sinica, 7, 180.Google Scholar
Florwski, D. R., et al., 1985, Astron. J., 90, 2381.CrossRefGoogle Scholar
Lestrade, J. F., et al., 1985, The Second F.A.S.T. Thinkshop, Marseille, Kovalevsky, J. (ed.), 87.Google Scholar
de Vegt, G., et al., 1985, Astron. J., 90, 2387.CrossRefGoogle Scholar
Schwan, H., 1985, Astron. Astrophys., 149, 50.Google Scholar