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• W2131707060 endingPage "504" @default.
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• W2131707060 abstract "Context.Relativistic outflows represent one of the best-suited tools to probe the physics of AGN. Numerical modelling of internal structure of the relativistic outflows on parsec scales provides important clues about the conditions and dynamics of the material in the immediate vicinity of the central black holes in AGN." @default.
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• W2131707060 date "2006-08-31" @default.
• W2131707060 modified "2023-10-17" @default.
• W2131707060 title "The role of Kelvin-Helmholtz instability in the internal structure of relativistic outflows. The case of the jet in 3C 273" @default.
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• W2131707060 doi "https://doi.org/10.1051/0004-6361:20065310" @default.
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