Traveling self-sustained structures in interstellar clouds with the isentropic instability
From MaRDI portal
Publication:416237
DOI10.1007/S10509-011-0683-0zbMath1237.85021OpenAlexW2043697474MaRDI QIDQ416237
R. N. Galimov, D. I. Zavershinsky, V. G. Makaryan, N. E. Molevich
Publication date: 9 May 2012
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10509-011-0683-0
Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20)
Related Items (3)
Magnetoacoustic heating in nonisentropic plasma caused by different kinds of heating-cooling function ⋮ Thermal self-action effects of acoustic beam in a vibrationally relaxing gas ⋮ Wave structures in ideal gas flows with an external energy source
Cites Work
- Structure and bifurcations of plane shock waves in a vibrationally excited gas with an external pumping source
- Structure of a gasdynamic disturbance in a thermodynamically nonequilibrium medium with a power-law relaxation model
- Self-sustained solitary waves in non-equilibrium media
- Expansion dynamics of volatile-supersaturated liquids and bulk viscosity of bubbly magmas
- A Method for the Numerical Calculation of Hydrodynamic Shocks
- Nonisothermal wave motions in the HII regions
This page was built for publication: Traveling self-sustained structures in interstellar clouds with the isentropic instability