No CrossRef data available.
Article contents
Comparison of Optical and Radio Positions of Stars
Published online by Cambridge University Press: 19 July 2016
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 positions of radio stars measured with respect to the VLBI network of extragalactic sources provides an important link between the optical and extragalactic reference frames. The establishment of this link was brought a stage nearer realization with the publication by Florkowski et al.(1985) of the radio positions of 20 stars measured with the Very Large Array (VLA) of the National Radio Astronomy Observatory, and the publication by Lestrade et al.(1985, 1988) of 10 stars measured with the VLBI network.
- Type
- Part 4: Realization and comparison of reference frames
- Information
- Symposium - International Astronomical Union , Volume 141: Inertial Coordinate System on the Sky , 1990 , pp. 513 - 514
- Copyright
- Copyright © Kluwer 1990
References
Florkowski, K.J., Johnston, K.J., Wade, C.M. & de Vegt, C. : (1985),
Astron. J.
90, 2381.Google Scholar
Johnston, K.J., de Vegt, C., Florkowski, D.R. & Wade, C.M. : (1985),
Astron. J.
90, 2390.CrossRefGoogle Scholar
Lestrade, J.-F., Preston, R.A., Requième, Y., Rapaport, M. and Mutel, R.L. : (1985), in
HIPPARCOS, Scientific Aspects of the Input Catalogue Preparation
, 251, ESA SP-234.Google Scholar
Lestrade, J.-F., White, G.L., Jauncey, D.L. and Preston, R.A. : (1988), in
HIPPARCOS, Scientific Aspects of the Input Catalogue Preparation II
, 481, Comissió Interdepartamental de Recerca i Innovació Tecnològica, Generalitat de Catalunya.Google Scholar
You have
Access