Effects of dense medium surrounding galactic-sized radio sources

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Astronomical Models, Cooling Flows (Astrophysics), Interstellar Magnetic Fields, Interstellar Matter, Polarization (Waves), Quasars, Radio Galaxies, Radio Jets (Astronomy), Stellar Spectra, Stellar Winds, Astronomical Interferometry, Magnetohydrodynamic Flow, Plasma Interactions, Radio Interferometers, Supersonic Jet Flow, Very Long Base Interferometry

Scientific paper

In this paper, I have analysed the subarcsecond polarization structure of two high-z compact steep-spectrum quasars. Morphology suggests that the jets are interacting strongly with intergalactic medium. Models of bending by ram pressure equilibrium in a cooling flow and alignment of magnetic field lines by jet-intergalactic medium (IGM) shock suggest that the compact steep-spectrum sources (CSS) jets are light, supersonic and mildly relativistic. Particle energy index variations along the jet suggests replenishment triggered by such interactions.

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