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Observations of Superluminal Motions in 3C 120

Walker, R. C. and Benson, J. M. and Seielstad, G. A. and Unwin, S. C. (1984) Observations of Superluminal Motions in 3C 120. In: VLBI and Compact Radio Sources. IAU Symposium Proceedings Series. No.110. D. Reidel , Dordrecht, pp. 121-124. ISBN 9789027717399. https://resolver.caltech.edu/CaltechAUTHORS:20181211-094921828

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Abstract

Superluminal motions were first seen in 3C 120 between 1972.5 and 1974.4 (Seielstad et al. 1979 and references therein). Between 1975 and 1980, the source was monitored along with 3C 273 and 3C 345 by the Caltech group. One reasonably clear episode of expansion was seen in 1979 (Walker et al. 1982) but, for most of the time, the source evolution was so rapid that it was difficult to relate the structures seen at successive epochs.


Item Type:Book Section
Related URLs:
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https://doi.org/10.1017/S0074180900077834DOIArticle
Additional Information:© 1984 by the IAU.
Series Name:IAU Symposium Proceedings Series
Issue or Number:110
Record Number:CaltechAUTHORS:20181211-094921828
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20181211-094921828
Official Citation:Walker, R., Benson, J., Seielstad, G., & Unwin, S. (1984). Observations of Superluminal Motions in 3C 120. Symposium - International Astronomical Union, 110, 121-124. doi:10.1017/S0074180900077834
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:91677
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:11 Dec 2018 18:00
Last Modified:03 Oct 2019 20:37

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