Traveling self-sustained structures in interstellar clouds with the isentropic instability

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

zbMATH Keywords

ISMShock wavesHydrodynamicsCloudsGeneralNegative viscosityThermal instabilities

Mathematics Subject Classification ID

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

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