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- W1659290410 abstract "Abstract The stability problem for a standing shock wave in an accretion flow on to a Newtonian point mass is considered. The linear perturbations are taken in the form e iwtYim, where ω is the frequency of the perturbations and l is the wavenumber of spherical harmonics. The eigenvalue describing the stability properties is determined by the finitness of the perturbed parameters of the flow at the sonic point. The shock front is unstable against radial perturbations for any adiabatic index 1 < γ < (5/3) and for any distance between the shock front and the sonic point. If this distance exceeds some critical value the mode l = 1 also becomes unstable." @default.
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- W1659290410 date "1999-08-01" @default.
- W1659290410 modified "2023-10-16" @default.
- W1659290410 title "Instability of spherical accretion with a shock wave on to a point mass" @default.
- W1659290410 cites W1982533270 @default.
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- W1659290410 doi "https://doi.org/10.1080/10556799908203052" @default.
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