Add to ORKGThe stability of a self-gravitating, nonrotating, plane-parallel, isothermal gas layer with equipartition magnetic and cosmic ray components, immersed in a rigid isothermal layer of stars, is considered with respect to waves with motions perpendicular to the equilibrium magnetic and gravitational field vectors. The magnetic field and cosmic ray gas hinder gravitational instability and increase the minimum length necessary to produce instability
Instabilities driven by some combination of rotation, velocity shear, and magnetic field in a strati...
We examine the consequences of treating a galactic disk as a two-fluid system for the stability of t...
We obtain the criterion for local stability against axisymmetric perturbations in gravitationally co...
A linear stability analysis of a multi-component and magnetized Galactic disk model is presented. Th...
Dynamic instability of interstellar gas caused by galactic cosmic rays and magnetic fiel
Purely gravitational perturbations are considered in a thin rotating disk composed of several gas an...
The influence of rotation and magnetic fields on the physical properties of isothermal gas clouds is...
Stability of simple equilibrium periodic system for interstellar gas and magnetic fiel
We model the Parker instability in vertically stratified isothermal gas using non-ideal MHD three-di...
Cold gas entering the central $1$ to $10^2$ pc of a galaxy fragments and condenses into clouds. The ...
Interstellar gas-cosmic radiation relationship for inflation of galactic magnetic field and halo pro...
A linear stability analysis has been performed onto a self-gravitating magnetized gas disk bounded b...
We perform a linear magnetohydrodynamic perturbation analysis for a stratified magnetized envelope w...
The generation of magnetohydrodynamic (MHD) waves and their instabilities are studied in galactic ga...
Large reservoirs of cold (~10⁴ K) gas exist out to and beyond the virial radius in the circumgalacti...
Instabilities driven by some combination of rotation, velocity shear, and magnetic field in a strati...
We examine the consequences of treating a galactic disk as a two-fluid system for the stability of t...
We obtain the criterion for local stability against axisymmetric perturbations in gravitationally co...
A linear stability analysis of a multi-component and magnetized Galactic disk model is presented. Th...
Dynamic instability of interstellar gas caused by galactic cosmic rays and magnetic fiel
Purely gravitational perturbations are considered in a thin rotating disk composed of several gas an...
The influence of rotation and magnetic fields on the physical properties of isothermal gas clouds is...
Stability of simple equilibrium periodic system for interstellar gas and magnetic fiel
We model the Parker instability in vertically stratified isothermal gas using non-ideal MHD three-di...
Cold gas entering the central $1$ to $10^2$ pc of a galaxy fragments and condenses into clouds. The ...
Interstellar gas-cosmic radiation relationship for inflation of galactic magnetic field and halo pro...
A linear stability analysis has been performed onto a self-gravitating magnetized gas disk bounded b...
We perform a linear magnetohydrodynamic perturbation analysis for a stratified magnetized envelope w...
The generation of magnetohydrodynamic (MHD) waves and their instabilities are studied in galactic ga...
Large reservoirs of cold (~10⁴ K) gas exist out to and beyond the virial radius in the circumgalacti...
Instabilities driven by some combination of rotation, velocity shear, and magnetic field in a strati...
We examine the consequences of treating a galactic disk as a two-fluid system for the stability of t...
We obtain the criterion for local stability against axisymmetric perturbations in gravitationally co...