We perform a normal mode analysis for nonaxisymmetric perturbations in a thin, differentially rotating disk with a vertical structure that is isothermal and convectively unstable. The vertical gravity is assumed to be external and constant. The perturbation scale is assumed to be much shorter than the radius of the disk but comparable to or less than the thickness. The initial value problem is formulated in shearing coordinates. Dispersion relations are obtained for the three limiting cases of zero shear, axisymmetric perturbations, and small radial wavelengths. The full effects of shear are studied by integrating numerically the initial value problem. The main results of the paper are as follows: (1) Nonaxisymmetric local Fourier modes hav...
Aims. We investigate whether differentially rotating regions of stellar radiative zones (such as the...
This paper discusses new perspectives and approaches to the problem of disk dynamics where, in this ...
This paper deals with the problem of hydrodynamic shear turbulence in non-magnetized Keplerian disks...
International audienceWe examine accretion disk flow under combined radial and vertical stratificati...
[[abstract]]We investigate Parker’s instability for a differentially rotating system comprised of th...
We discuss the possibility that astrophysical accretion disks are dynamically unstable to non-axisy...
We discuss the possibility that astrophysical accretion disks are dynamically unstable to non-axisym...
. Global modes of the magnetic shear instability in horizontally unbounded rotating disks are studie...
We present a study of instabilities occuring in thick magnetized accretion disks. We calculate the g...
We consider the stability properties of discs rotating with the angular velocity dependent on both ...
We carry out a general study of the stability of astrophysical flows that appear steady in a uniform...
This is a sequel to Paper I (Chagelishvili et al. 2003), where we presented the so-called bypass con...
This work presents a linear analytical calculation on the stability and evolution of a compressible,...
The hydrodynamic stability of accretion disks is considered. The particular question is whether the...
Protoplanetary discs, composed of gas and dust, usually surround young stellar objects and serve two...
Aims. We investigate whether differentially rotating regions of stellar radiative zones (such as the...
This paper discusses new perspectives and approaches to the problem of disk dynamics where, in this ...
This paper deals with the problem of hydrodynamic shear turbulence in non-magnetized Keplerian disks...
International audienceWe examine accretion disk flow under combined radial and vertical stratificati...
[[abstract]]We investigate Parker’s instability for a differentially rotating system comprised of th...
We discuss the possibility that astrophysical accretion disks are dynamically unstable to non-axisy...
We discuss the possibility that astrophysical accretion disks are dynamically unstable to non-axisym...
. Global modes of the magnetic shear instability in horizontally unbounded rotating disks are studie...
We present a study of instabilities occuring in thick magnetized accretion disks. We calculate the g...
We consider the stability properties of discs rotating with the angular velocity dependent on both ...
We carry out a general study of the stability of astrophysical flows that appear steady in a uniform...
This is a sequel to Paper I (Chagelishvili et al. 2003), where we presented the so-called bypass con...
This work presents a linear analytical calculation on the stability and evolution of a compressible,...
The hydrodynamic stability of accretion disks is considered. The particular question is whether the...
Protoplanetary discs, composed of gas and dust, usually surround young stellar objects and serve two...
Aims. We investigate whether differentially rotating regions of stellar radiative zones (such as the...
This paper discusses new perspectives and approaches to the problem of disk dynamics where, in this ...
This paper deals with the problem of hydrodynamic shear turbulence in non-magnetized Keplerian disks...