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Instabilities in astrophysical jets

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Abstract

The observed properties of astrophysical jets are reviewed, and the techniques used to estimate the parameters of the underlying beams are described. This information is then used in a theoretical treatement of the Kelvin-Helmholtz instability of the flows, and the relevance of this instability to the persistence of the observed structures is emphasised.

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  1. M. Birkinshaw

    Present address: Smithsonian Astrophysical Observatory, 60 Garden Street, 02138, Cambridge, MA, USA

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    M. Birkinshaw

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Birkinshaw, M. Instabilities in astrophysical jets. Astrophys Space Sci 242, 17–91 (1996). https://doi.org/10.1007/BF00645111

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