Polarization Observations of Radio Sources in the Field Containing Abell 695

Details Polarization Observations of Radio Sources in the Field Containing Abell 695 Polarization Observations of Radio Sources in the Field Containing Abell 695

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jkas...21..117k&link_type=abstract

Journal of the Korean Astronomical Society, vol. 21, p. 117-132

Astronomy and Astrophysics

Astronomy

Scientific paper

Multi-frequency polarization observations of Abell 695 are reported here. The brightest radio source 0838+325, which was previously classified as a wide angled head-tail radio source, is, in the present observations, resolved into two separable sources, a head-tail source 0838+325 AB and a diffuse one 0838+325C. The radio-tail shows high degree of linear polarization (~50-25%) along the radio-tail, suggesting that the interaction with its surrounding intracluster medium (ICM) is not highly turbulent. With the present data, thermal particle densities at the locations of these sources are estimated to be n > 10e-5 /cm3.

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