The tail of 3C 129 - Observations at 2.7 GHz

Details The tail of 3C 129 - Observations at 2.7 GHz The tail of 3C 129 - Observations at 2.7 GHz

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.211..215d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 211, Nov. 1, 1984, p. 215-220. Research supported by th

Astronomy and Astrophysics

Astronomy

11

Extragalactic Radio Sources, Magnetic Field Configurations, Polarized Radiation, Radio Galaxies, Radio Spectra, Flux Density, Radio Astronomy, Radio Sources (Astronomy)

Scientific paper

Observations of the tailed radio galaxy 3C129 at 2.7 GHz with an angular resolution of 4.3 arcmin are presented. These observations allow the outer regions of the tail to be investigated. The tail is shorter than at low frequencies because of spectral steepening, and shows polarization as strong as 50 per cent of the total power. The magnetic field lies along the tail.

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