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The Parsec-Scale Radio Polarization of Three GHz-Peaked–Spectrum Radio Sources

Published online by Cambridge University Press:  12 April 2016

C. Stanghellini ,
D. Dallacasa ,
C.P. O’Dea ,
S.A. Baum ,
C. Fanti  and
R. Fanti
C. Stanghellini
Affiliation:
Istituto di Radioastronomia del C.N.R., Italy
D. Dallacasa
Affiliation:
Istituto di Radioastronomia del C.N.R., Italy
C.P. O’Dea
Affiliation:
Space Telescope Science Institute, Baltimore, MB, U.S.A.
S.A. Baum
Affiliation:
Space Telescope Science Institute, Baltimore, MB, U.S.A.
C. Fanti
Affiliation:
Dipartimento di Fisica, Univ. Bologna, Bologna, Italy
R. Fanti
Affiliation:
Dipartimento di Fisica, Univ. Bologna, Bologna, Italy

Abstract

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Preliminary results on the parsec-scale polarization properties at 15 GHz of 3 GHz-peaked-spectrum radio sources are presented.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 177 - 178
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Fanti, C., et al. 1995. A&A, 302, 317–326.Google Scholar
Phillips, R.B., & Mutel, R.L. 1982. A&A, 106, 21–24.Google Scholar
Readhead, A.C.S., et al. 1996. ApJ, 460, 634–643.Google Scholar
Stanghellini, C., et al. 1996. In The Second Workshop on Gigahertz Peaked Spectrum and Compact Steep Spectrum Radio Sources, eds. Snellen, I.A.G. et al. (Leiden: Leiden Observatory), 4–13.Google Scholar
van Breugel, W., Miley, G., & Heckman, T. 1984. AJ, 89, 5–22.Google Scholar