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- W1785351036 abstract "Using the anelastic approximation of linearised hydrodynamic equations, we investigate the development of axially symmetric small perturbations in thin Keplerian discs. The sixth-order dispersion equation is derived and numerically solved for different values of relevant physical parameters (viscosity, heat conductivity, disc semi-thickness and vertical structure). The analysis reveals the appearance of two overstable modes which split out from the classical Rayleigh inertial modes in a wide range of the parameters in both ionized and neutral gases. These modes have a viscous-convective nature and can serve as a seed for turbulence in astrophysical discs even in the absence of magnetic fields." @default.
- W1785351036 created "2016-06-24" @default.
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- W1785351036 date "2015-06-30" @default.
- W1785351036 modified "2023-10-17" @default.
- W1785351036 title "A viscous–convective instability in laminar Keplerian thindiscs – II. Anelastic approximation" @default.
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- W1785351036 doi "https://doi.org/10.1093/mnras/stv1246" @default.
- W1785351036 hasPublicationYear "2015" @default.
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