Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-30T02:53:22.454Z Has data issue: false hasContentIssue false
  • English
  • Français

Superluminal Motion of 3C273B and the Apparent Right Ascension Shift

Published online by Cambridge University Press:  03 August 2017

N. Kawaguchi  and
Y. Takahashi
N. Kawaguchi
Affiliation:
Kashima Space Research Center, Radio Research Laboratory, 893-1, Hirai, Kashima, Ibaraki 314, Japan
Y. Takahashi
Affiliation:
Kashima Space Research Center, Radio Research Laboratory, 893-1, Hirai, Kashima, Ibaraki 314, Japan

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 effect of the superluminal motion of 3C273b was observed on the fringe amplitudes obtained in VLBI experiments which have been conducted on the baselines between Japan and United States since 1984 under the Crustal Dynamics Project. The speed was 0.7 mas/year and the direction was −83 degrees in the position angle. It was also confirmed as the apparent right ascention shift of the source.

Type
Extragalactic
Information
Symposium - International Astronomical Union , Volume 129: The Impact of VLBI on Astrophysics and Geophysics , 1988 , pp. 45 - 46
Copyright
Copyright © Reidel 1988 

References

[1] Unwin, S.C., et al. 1985, Ap. J., 289, 109 CrossRefGoogle Scholar