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A Multi-Frequency VLBI Polarization Study of the CSS Quasar 3C 309.1
Published online by Cambridge University Press: 12 April 2016
Abstract
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We discuss the rotation measure properties of the CSS quasar 3C 309.1, determined from high dynamic range, large field of view VLBA images at several frequencies between 1.4 and 15 GHz. We consider the general properties of the ambient medium by considering the structure of the Faraday screen across various parts of the radio source.
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- Research Article
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- Copyright © Astronomical Society of the Pacific 1998
References
Aaron, S.E., Wardle, J.F.C., & Roberts, D.H.
1997. Vistas in Astronomy, Vol. 41, No. 2, ed. Colomer, F. & Garrett, M., 225–229 (AWR97).Google Scholar
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