Normal modes of Bardeen discs - I. Uniformly rotating incompressible discs

DOI10.1093/MNRAS/202.3.867zbMath0524.76051OpenAlexW2088110328MaRDI QIDQ3036968

Alison M. Bowen, Bernard F. Schutz

Publication date: 1983

Published in: Monthly Notices of the Royal Astronomical Society (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1093/mnras/202.3.867

zbMATH Keywords

stellar modelsself-gravitationapproximation to Maclaurin spheroidsBardeen approximationeffects of gravitational radiation and viscosity on spectrumrotation pressuresequence of uniformly rotating incompressible fluid discs

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Interfacial stability and instability in hydrodynamic stability (76E17) Hydrodynamic stability (76E99) Galactic and stellar dynamics (85A05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20)

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