K.C. Chambers (1), G.K. Miley (2), W.J.M. van Breugel (3), M.A.R. Bremer (2,4), J. Huang (1), N. Trentham (1)
1 Institute for Astronomy, University of Hawaii
2 Sterrewacht Leiden
3 Institute for Geophysics and Planetary Physics, Lawrence Livermore
National Laboratory
4 Space Research Organisation of the Netherlands, Utrecht
ABSTRACT
We present radio, infrared, optical, and HST imaging data on eight high
redshift () ultra steep spectrum 4C radio sources. The radio polarization
morphologies are highly asymmetric. The optical morphologies are all aligned
with the radio axis. The multi-color images show strong asymmetric gradients
in the color of the continuum along the radio axes. No optical emission is
detected from the radio lobes. Narrow band images of the redshifted Lyman
emission show that the emission line morphology is generally
aligned with the radio source but does not necessarily correlate
with the apparent morphology of the rest frame ultraviolet continuum.
Subject headings: radio sources: identifications - radio sources: galaxies - galaxies: redshifts
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