Magnetic Fields in Clusters: Faraday Rotation in
A400 and A2634
J.A. Eilek1
, F.N. Owen2
We present Faraday rotation data for radio sources
in the centers of the Abell clusters A400 and A2634. These clusters
do not contain strong cooling cores, while they do contain large
(>100 kpc), tailed radio sources. Thus, our data extend
previous work on rotation measure in cluster centers, to lower density
cores, and larger scales.
Radio contours of 3C465, overlaid on ROSAT X-ray image
of inner part of A2634
We find the rotation measure, and thus the
magnetic field, is ordered on scales ~10-20 kpc in both
clusters; and its geometry appears to be determined by the
distribution of the X-ray emitting gas, rather than by the radio
tails.
Radio contours of 3C75, overlaid on ROSAT X-ray image
of inner part of A400
We also find the magnetic fields in these
clusters are dynamically important, We suggest that these as well
as previous cluster-center Faraday data are measuring magnetic fields in the
intracluster medium, rather than in a skin of the radio source.

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