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Supersonic Jets and Lobe Morphologies

Published online by Cambridge University Press:  25 May 2016

A. Ferrari
Affiliation:
Dipartimento di Fisica Generale, Università di Torino Via P. Giuria 1, I–10125 Torino, Italy Osservatorio Astronomico di Torino Strada dell'Osservatorio 20, 10025 Pino Torinese, Italy
S. Massaglia
Affiliation:
Dipartimento di Fisica Generale, Università di Torino Via P. Giuria 1, I–10125 Torino, Italy Osservatorio Astronomico di Torino Strada dell'Osservatorio 20, 10025 Pino Torinese, Italy
G. Bodo
Affiliation:
Dipartimento di Fisica Generale, Università di Torino Via P. Giuria 1, I–10125 Torino, Italy Osservatorio Astronomico di Torino Strada dell'Osservatorio 20, 10025 Pino Torinese, Italy

Extract

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Since the pioneering work by Norman et al. (1982), many numerical studies have been devoted to the analysis of the propagation of a supersonic jet shot into an ambient medium (see Massaglia, Bodo & Ferrari 1995, hereinafter Paper I, and references therein). In spite of these strong efforts many aspects of this problem are still not well understood. This is due to the complexity of the jet-cocoon structure: in fact, the cocoon excites perturbations to the jet flow, which in turn can be amplified by the Kelvin–Helmholtz mechanism and induce a strong activity of the jet's head that affects the cocoon structure. Thus a complex feedback loop mechanism establishes between jet and cocoon which make the dynamics of the interaction very complex.

Type
Radio Source Modelling and Emission Mechanisms
Copyright
Copyright © Kluwer 1996 

References

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Massaglia, S., Bodo, G., Ferrari, A.: A&A (Paper I) in press (1995)Google Scholar
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