Structure of accretion flow in close binary system: A two dimensional numerical model

Details Structure of accretion flow in close binary system: A two dimensional numerical model Structure of accretion flow in close binary system: A two dimensional numerical model

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.311..255d&link_type=abstract

In ESA, Plasma Astrophysics p 255-260 (SEE N91-15046 06-90)

Astronomy and Astrophysics

Astrophysics

Accretion Disks, Astronomical Models, Binary Stars, Cosmic Gases, Gas Dynamics, Gas Flow, Mathematical Models, Shock Fronts, Density Distribution, Equations Of Motion, Lagrangian Equilibrium Points, Magnetic Fields, Two Dimensional Models

Scientific paper

A two dimensional numerical model forming two spiral shock fronts in accretion flow in close binary star system is presented. The position of these shocks is discussed. In the model, the position of the second shock front depends on the relation between the masses of both stars and the distance between them. Experimental computation based on smaller mass of the second star reveals closer position of the second spiral to the first one.

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