Hostname: page-component-77c89778f8-fv566 Total loading time: 0 Render date: 2024-07-18T13:29:08.783Z Has data issue: false hasContentIssue false
  • English
  • Français

Residual rotation of the FK5 from optical observations of the planets 1960–1994

Published online by Cambridge University Press:  25 May 2016

Yu. B. Kolesnik
Yu. B. Kolesnik*
Affiliation:
Institute for Astronomy of the Russian Academy of Sciences, 109017,48 Piatnitskaya St., Moscow, Russia

Extract

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.

In the interval covering last three decades optical observations of the Sun and major planets have been produced with an unprecedented intensity. Most of the published world-wide observations of the Sun, Mercury, Venus and Mars made from 1960 to 1994 with transit circles, astrographs and astrolabes are incorporated here for investigation of the residual rotation of the stellar system with respect to the dynamical reference frame.

Type
Part XI - Reference Frames. Stellar Astrometry
Information
Symposium - International Astronomical Union , Volume 172: Dynamics, Ephemerides and Astrometry of the Solar System , 1996 , pp. 477 - 480
Copyright
Copyright © Kluwer 1996 

References

Fukushima, T., 1991, in Hugues, J.A., Smith, C.A., Kaplan, G.H. (eds) Reference Systems, USNO, Washington, p.27 Google Scholar
Kolesnik, Yu.B., 1995, A & A 294, 876 Google Scholar
Kolesnik, Yu.B., 1996, submitted to MNRAS Google Scholar
Schwan, H., 1988, A & A 198, 116 Google Scholar
Standish, E.M., Williams, J.G., 1990, in Lieske, J.H. and Abalakin, V.K. (eds.) Inertial Coordinate System on the Sky, Kluwer, Dordrecht, p.173 CrossRefGoogle Scholar
Sveshnikov, M.L., 1972, Bull. ITA 13,131 (in Russian) Google Scholar