Nonlinear phenomena in accretion disks: Possibility for observational verification

Details Nonlinear phenomena in accretion disks: Possibility for observational verification Nonlinear phenomena in accretion disks: Possibility for observational verification

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..409f&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 409-413 (SEE N90-25711 19-89)

Mathematics

Dynamical Systems

Accretion Disks, Nonlinear Systems, Stellar Evolution, Viscosity, Angular Momentum, Dynamical Systems, Stellar Mass Accretion, Stellar Physics, Stellar Rotation

Scientific paper

The behavior of the accretion disk is investigated. Equations in variables of the momentum friction force between two adjacent cylinders and the specific angular momentum are used. A few exact solutions are found. A scenario for the evolution of the accretion disk is suggested. The possibilities for the construction of a theory describing the global properties of the accretion disk with viscosity as a main parameter are discussed.

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