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Evolution of the Milliarcsecond Polarization Structure of the Superluminal Quasar 3C345

Published online by Cambridge University Press:  03 August 2017

J. F. C. Wardle ,
D. H. Roberts ,
L. F. Brown  and
D. C. Gabuzda
J. F. C. Wardle
Affiliation:
Department of Physics, Brandeis University, Waltham, MA 02254 USA
D. H. Roberts
Affiliation:
Department of Physics, Brandeis University, Waltham, MA 02254 USA
L. F. Brown
Affiliation:
Department of Physics, Brandeis University, Waltham, MA 02254 USA
D. C. Gabuzda
Affiliation:
Department of Physics, Brandeis University, Waltham, MA 02254 USA

Abstract

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The λ6 cm milliarcsecond polarization structure of 3C345 has been determined at three epochs between December 1981 and March 1984. The knots C2, C3, and C4 all showed changes as they moved away from the core, which remained virtually unpolarized.

Type
Extragalactic
Information
Symposium - International Astronomical Union , Volume 129: The Impact of VLBI on Astrophysics and Geophysics , 1988 , pp. 163 - 164
Copyright
Copyright © Reidel 1988 

References

Biretta, J. A., Moore, R. L., and Cohen, M. H. 1986, Astrophys. J., 308, 93–109.Google Scholar
Roberts, D. H., et al., 1984, in VLBI and Compact Radio Sources, ed. Fanti, R., Kellermann, K., and Setti, G. (Dordrecht: Reidel), 35–38.CrossRefGoogle Scholar
Wardle, J. F. C., Roberts, D. H., Potash, R. I., and Rogers, A. E. E. 1986, Astrophys. J. (Letters), 304, L1–L4.Google Scholar