Hostname: page-component-5cf477f64f-bmd9x Total loading time: 0 Render date: 2025-04-07T02:31:59.637Z Has data issue: false hasContentIssue false
  • English
  • Français

Asymmetric Depolarization in Double Radio Sources

Published online by Cambridge University Press:  19 July 2016

S. T. Garrington ,
R. G. Conway  and
G. F. Holmes
S. T. Garrington
Affiliation:
Nuffield Radio Astronomy Laboratories Jodrell Bank Macclesfield, Cheshire SK11 9DL, U.K.
R. G. Conway
Affiliation:
Nuffield Radio Astronomy Laboratories Jodrell Bank Macclesfield, Cheshire SK11 9DL, U.K.
G. F. Holmes
Affiliation:
Nuffield Radio Astronomy Laboratories Jodrell Bank Macclesfield, Cheshire SK11 9DL, U.K.

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.

The asymmetric depolarization seen in powerful extragalactic double sources with one sided jets may be explained in terms of differential Faraday effects in a halo of gas surrounding the source, provided the halo has a core-radius ~30–100 kpc, and contains a magnetic field of order >1 μGauss tangled on a scale <5 kpc.

Type
9. Magnetic Fields in the Galactic Environment, Galaxy Clusters and Intergalactic Medium
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 473 - 476
Copyright
Copyright © Kluwer 1990 

References

Burn, B.J., 1986. Mon. Not. R. astr. Soc., 133, 67.CrossRefGoogle Scholar
Garrington, S.T., Leahy, J.P., Conway, R.G. and Laing, R.A., 1988. Nature 331, 147.Google Scholar
Sarazin, C.L., 1986. Rev. Mod. Phys. 58, 1.Google Scholar
Schwartz, D.A., Schwarz, J. and Tucker, W., 1980. Astrophys. J. 238,L59.Google Scholar
Strom, R.G., 1973. Astr. Astrophys., 25, 303.Google Scholar