Particle simulation for accretion sheets in narrow double stars

Details Particle simulation for accretion sheets in narrow double stars Particle simulation for accretion sheets in narrow double stars

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988cpp..conf...90g&link_type=abstract

In Max-Planck-Inst. für Physik und Astrophysik, Cosmic Plasma Physics p 90-97 (SEE N89-25716 19-75)

Physics

Plasma Physics

1

Cosmic Plasma, Double Stars, Dynamic Characteristics, Particle Interactions, Simulation, Stellar Mass Accretion, Friction, Particle Motion, Viscosity, Viscous Drag

Scientific paper

Development and behavior of accretion sheets in double stars systems are studied by particle simulation calculations. Numerical analysis considers the following parameters in the binary system: primary and secondary components, path period of the system, and mass flow rates. Mass behavior is described by Roche-potential. The particle motion equation in the double star system is solved by the Leap-Frog procedure. Velocity friction simulation is obtained by viscous interaction considerations.

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