Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-27T04:41:33.895Z Has data issue: false hasContentIssue false

A Multi-Frequency VLBI Polarization Study of the CSS Quasar 3C 309.1

Published online by Cambridge University Press:  12 April 2016

Scott E. Aaron
Affiliation:
Max-Planck-Institut für Radioastronomie, 53121 Bonn, Germany
John F.C. Wardle
Affiliation:
Department of Physics, Brandeis University, Waltham, MA 02254, U.S.A.
David H. Roberts
Affiliation:
Department of Physics, Brandeis University, Waltham, MA 02254, U.S.A.

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.

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.

Type
Research Article
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Aaron, S.E. 1996. Ph.D. Thesis, Brandeis University.Google Scholar
Aaron, S.E., Wardle, J.F.C., & Roberts, D.H. 1997. Vistas in Astronomy, Vol. 41, No. 2, ed. Colomer, F. & Garrett, M., 225229 (AWR97).Google Scholar
Fanti, C., et al. 1985. A&A, 143, 292306.Google Scholar
Forbes, D.A., et al. 1990. MNRAS, 244, 680690.Google Scholar
Taylor, G.B., Barton, E.J., & Ge, J.P. 1994. AJ, 107, 19421952.Google Scholar
van Breugel, W., Miley, G., & Heckman, T. 1984. AJ, 89, 522.Google Scholar