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X-Band VLBA Polarization of 3C 287

Published online by Cambridge University Press:  12 April 2016

D. Dallacasa ,
R. T. Schilizzi  and
Nan Rendong
D. Dallacasa
Affiliation:
Istituto di Radioastronomia, CNR, Bologna, Italy
R. T. Schilizzi
Affiliation:
Joint Institute for VLBI in Europe, Dwingeloo, The Netherlands
Nan Rendong
Affiliation:
Beijing Radio Observatory, Beijing, China

Abstract

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VLBA polarimetric observations at 8.15 and 8.54 GHz of the quasar 3C 287 are presented and discussed. The source structure is complex, and the magnetic field geometry does not help in the interpretation of the source.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 117 - 118
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Fanti, C., et al. 1989. A&A, 217, 44–56.Google Scholar
Fanti, C., et al. 1995. A&A, 302, 317–326.Google Scholar
Readhead, A.C.S., et al. 1996. Ap], 460, 634–643.Google Scholar
van Breugel, W., Miley, G., & Heckman, T. 1984. AJ, 89, 5–22.Google Scholar