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- W33453309 abstract "Des instabilites de Kelvin-Helmholtz dans une configuration a symetrie axiale produisent une relation de dispersion qui peut etre resolue avec une routine numerique lorsque les longueurs d'ondes sont plus courtes que le rayon du jet. On utilise le taux de croissance dans une approche en cascade turbulente pour expliquer la luminosite du jet" @default.
- W33453309 created "2016-06-24" @default.
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- W33453309 date "1985-07-01" @default.
- W33453309 modified "2023-09-26" @default.
- W33453309 title "Relativistic short wavelength instabilities in astrophysical jets. I: Fluidodynamical case" @default.
- W33453309 hasPublicationYear "1985" @default.
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