Analytical Modeling of Infant Radio Sources

Physics

Scientific paper

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X-Ray, Radio, Dissipation Of Jets

Scientific paper

We extend previous analytical models of FRII-type radio source growth to model very young sources. The new model describes the source evolution in the regime before self-similarity and when ballistic growth of the jet must be considered. Dynamical and spectral results are given showing the evolution from a highly over-dense jet which punches its way forward through the surrounding medium to the stage where its progress is slowed by the surroundings and the cocoon begins to inflate. We follow the source evolution by calculating the synchrotron emissivity and the frequency at which the spectrum peaks at various stages of growth.

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