Hostname: page-component-77c89778f8-gq7q9 Total loading time: 0 Render date: 2024-07-22T17:04:10.227Z Has data issue: false hasContentIssue false

Peculiar Magnetic Field Structures in 4C49.22 (1150+497)

Published online by Cambridge University Press:  19 July 2016

Chidi E. Akujor*
Affiliation:
Astrophysics Group, Department of Physics and Astronomy University of Nigeria Nsukka, Nigeria

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 present radio polarisation observations of the quasar 4C49.22. It shows no evidence of depolarisation on the counter–jet side, while exhibiting strong variation of fractional polarisation along the jet, as well as transverse offset of maximum fractional polarisation from each knot in the jet.

Type
8. The Role of Magnetic Fields in Radio Source Jets and Extended Radio Lobes
Copyright
Copyright © Kluwer 1990 

References

Burns, B.J. et al. (1984) in Bridle, A.H. and Eilek, J.A. (eds.), Physics of Energy Transport in EGRSs, p. 255.Google Scholar
Garrington, S.T. et al. (1988) Nature 331, 147.CrossRefGoogle Scholar
Königl, A. and Choudhuri, A.R. (1985), Astrophys. J. 289, 173.CrossRefGoogle Scholar
Laing, R.A. (1981) Astrophys. J. 248, 87.CrossRefGoogle Scholar
Laing, R.A. (1988) Nature 331, 149.CrossRefGoogle Scholar
Laing, R.A. (1984) in Bridle, A.H. and Eilek, J.A. (eds.), Physics of Energy Transport in EGRSs, p. 90.Google Scholar
Strom, R.G. (1973) Astron. Astrophys. 25, 303.Google Scholar
Tabara, H. and Inoue, M. (1980) Astron. Astrophys. Suppl. 39, 379.Google Scholar