Non linear waves in two dimensional keplerian flows

DOI10.1080/03091928708210106zbMath0618.76039OpenAlexW1978286753WikidataQ114640345 ScholiaQ114640345MaRDI QIDQ3755074

No author found.

Publication date: 1987

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1080/03091928708210106

zbMATH Keywords

rotationperturbationsgravitational potentialshearingdynamical stabilityelectromagnetic radiationgravitational binding energyAccretion discstwo-dimensional supersonic Keplerian flow

Mathematics Subject Classification ID

Galactic and stellar dynamics (85A05) Statics (70C20) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Basic methods in fluid mechanics (76M99) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

• Unnamed Item
• The dynamical stability of differentially rotating discs with constant specific angular momentum
• Determining modes and fractal dimension of turbulent flows

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