Hostname: page-component-7479d7b7d-c9gpj Total loading time: 0 Render date: 2024-07-12T04:28:32.468Z Has data issue: false hasContentIssue false
  • English
  • Français

Contribution des Astrolabes au Raccordement des Systemes de Reference “Optique” et “Radio”.

Published online by Cambridge University Press:  12 April 2016

Suzanne Débarbat
Suzanne Débarbat*
Affiliation:
Observatoire de Paris, Paris, France

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.

Twenty-two radio sources, being bright objects of the Galaxy are observable with astro labe (plus six for those having photoelectric devices). It is about half of the total number (forty-six, figure 2) of objects of the list of galactic objects given by the working group of Commission six of the IAU. Seventeen astro labe stations (figure 2) are interested in a cooperation which final objective is to link the radio and optical reference systems.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 56: Reference Coordinate Systems for Earth Dynamics , August 1980 , pp. 363 - 367
Copyright
Copyright © Reidel 1981

References

Billaud, G.: 1978, Thèse, Contribution de l’astrolabe à l’amélioration du système fondamental de référence: le Catalogue Général.Google Scholar
Débarbat, S.: 1978, Colloque UAI n° 48.Google Scholar
Elsmore, B., Ryle, M.: 1976, MNRAS, 174, 411.Google Scholar
Johnston, K.J., Spencer, J.H., Kaplan, G.M., Klepczynski, W.J. and McCarthy, D.D.: 1980, Cel. Mech., 22.Google Scholar
Réquième, Y.: 1979, Colloque du GS V, Publication de l’Observatoire de Bordeaux.Google Scholar
Tucker, R.H., Yallop, B.D., Argue, A.N., Kenworthy, C.M., Elsmore, B. and Ryle, M.: 1973, MN3AS, 164, 27.Google Scholar
Vegt (de), Chr. and Gehlich, U.K.: 1978, Colloque UAI n° 48.Google Scholar
Wade, C.M., and Johnston, K.J.: 1977, Astron. J., 82, 791.Google Scholar
Walter, H.G. and West, R.M.: 1980, Astron. Astrophys., 86, 1.Google Scholar