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Instability of the celestial reference frame and effect on UT1
Published online by Cambridge University Press: 21 October 2010
Abstract
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It was shown that the ICRF radio sources including the defining sources have significant apparent motion that leads to rotation of the ICRF. This rotation is transformed to secular variations of EOP that is decreased or removed if motion of sources is took into account.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 209
- Copyright
- Copyright © International Astronomical Union 2010
References
Zharov, V. E., Sazhin, M. V., Sementsov, V. N., Kuimov, K. V., & Sazhina, O. S. 2009, Astr. Rep., 53, 579CrossRefGoogle Scholar