Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-24T14:16:50.308Z Has data issue: false hasContentIssue false

Instability of the celestial reference frame and effect on UT1

Published online by Cambridge University Press:  21 October 2010

Vladimir E. Zharov*
Affiliation:
Department of Physics, Moscow State University, Moscow, Russia email: [email protected]
Rights & Permissions [Opens in a new window]

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.

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.

Type
Contributed Papers
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
Zharov, V. E. 2009, submitted to Astr. Rep.Google Scholar
Ma, C., Arias, E. F., Eubanks, T. M., et al. , 1998, AJ, 116, 516CrossRefGoogle Scholar