The structure and stability of the accretion disc boundary layer

Details The structure and stability of the accretion disc boundary layer The structure and stability of the accretion disc boundary layer

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.220..593p&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 220, June 1, 1986, p. 593-610.

Astronomy and Astrophysics

Astronomy

95

Accretion Disks, Boundary Layer Stability, Magnetohydrodynamic Stability, Stellar Models, Stellar Structure, Perturbation Theory, Steady State, Stellar Oscillations, Viscosity

Scientific paper

An axially-symmetric accretion disc is treated both analytically and
numerically, with special attention paid to the boundary layer. A
modified form of the standard viscosity model is used. The authors show
the mechanism by which overstable oscillations can evolve there and how
they dissipate.

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