Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-26T19:34:01.571Z Has data issue: false hasContentIssue false
  • English
  • Français

The FK4 Orientation Parameters Derived From Photographic and VLBI Observations of Radio / Optical Objects

Published online by Cambridge University Press:  19 July 2016

V.S. Gubanov ,
I.I. Kumkova  and
N.I. Solina
V.S. Gubanov
Affiliation:
Institute of Applied Astronomy 8 Zhdanovskaya ul. 197042 Leningrad USSR
I.I. Kumkova
Affiliation:
Institute of Applied Astronomy 8 Zhdanovskaya ul. 197042 Leningrad USSR
N.I. Solina
Affiliation:
Institute of Applied Astronomy 8 Zhdanovskaya ul. 197042 Leningrad USSR

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 photographic and VLBI positions of 59 quasars are used for determination of the FK4 orientation parameters with respect to the radioastrometrical system (RAS).

Type
Part 2: Pulkovo today
Information
Symposium - International Astronomical Union , Volume 141: Inertial Coordinate System on the Sky , 1990 , pp. 85 - 86
Copyright
Copyright © Kluwer 1990 

References

1. Torres, C., Wrobiewski, H. : 1987, Astron. Astrophys. Suppl Ser. 69, 23.Google Scholar
2. Walter, H., West, R. : 1986, Astron. Astrophys. 156, 1.Google Scholar
3. Clements, E. : 1983, Monthly Notices Roy. Astron. Soc. 203, 861.Google Scholar
4. Argue, A.N., et al. : 1984, Astron. Astrophys. 130, 191.Google Scholar