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Interaction of jets with the ISM of radio galaxies

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Abstract

We present three dimensional simulations of the interaction of a light hypersonic jet with an inhomogeneous thermal and turbulently supported disk in an elliptical galaxy. These simulations are applicable to the GPS/CSS phase of some extragalactic radio sources.

We identify four generic phases in the evolution of such a jet with the interstellar medium. The first is a “flood and channel” phase, dominated by complex jet interactions with the dense cloudy medium close to the nucleus. This is characterized by high pressure jet gas finding changing weak points in the ISM and flowing through channels that form and reform over time. A spherical, energy driven, bubble phase ensues, wherein the bubble is larger than the disk scale, but the jet remains fully disrupted close to the nucleus, so that the jet flux is thermalised and generates a smooth isotropic energy-driven bubble. In the subsequent, rapid, jet break-out phase the jet breaks free of the last obstructing dense clouds, becomes collimated and pierces the more or less spherical bubble. In the final classical phase, the jet propagates in a momentum-dominated fashion similar to jets in single component hot haloes, leading to the classical jet–cocoon–bow-shock structure.

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Authors and Affiliations

  1. Research School of Astronomy & Astrophysics, Australian National University, Cotter Rd., Weston, ACT, 2611, Australia

    Ralph S. Sutherland & Geoffrey V. Bicknell

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  1. Ralph S. Sutherland
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  2. Geoffrey V. Bicknell
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Correspondence to Ralph S. Sutherland.

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Sutherland, R.S., Bicknell, G.V. Interaction of jets with the ISM of radio galaxies. Astrophys Space Sci 311, 293–303 (2007). https://doi.org/10.1007/s10509-007-9580-y

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  • DOI: https://doi.org/10.1007/s10509-007-9580-y

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