Extensive gaseous haloes surrounding giant elliptical galaxies - Evidence from depolarization in radio galaxies

Astronomy and Astrophysics – Astronomy

Scientific paper

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Depolarization, Elliptical Galaxies, Faraday Effect, Halos, Radio Galaxies, Electron Density (Concentration), Interstellar Magnetic Fields, Radio Telescopes, X Ray Astronomy

Scientific paper

Radio polarization measurements have been used to investigate large scale gaseous components associated with some thirteen double radio sources. At 49 cm a significant proportion of the bridge emission, roughly centered on the parent galaxy, is invariably found to be unpolarized. The authors present evidence that this lack of polarization at long wavelengths is the result of differential Faraday rotation in a large scale halo associated with the central (usually elliptical) galaxy. The haloes, which extend beyond 100 kpc, appear to be the outer envelopes of hot gas such as that observed in the form of extended X-ray emission associated with a number of nearby early-type galaxies.

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