Simulation of accretion disks due to viscosity in semi-detached binary systems

Details Simulation of accretion disks due to viscosity in semi-detached binary systems Simulation of accretion disks due to viscosity in semi-detached binary systems

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.134...25z&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 134, no. 1, June 1987, p. 25-34. Research supported by the China State Edu

Statistics

Computation

Accretion Disks, Binary Stars, Computational Astrophysics, Motion Simulation, Viscosity, Difference Equations, Equilibrium Flow, Mass Transfer, Particle Motion, Roche Limit

Scientific paper

A computation simulation of the motion of equilibrium particles in semi-detached binary systems is presented. The author finds that an accretion disk can be formed around the primary due to viscosity between moving particles. The calculated results are obtained for various factors and mass ratios. The results show that a part of the matter transferred from the secondary is accreted by the primary and the equilibrium mass transfer of moving particle depends on viscous factors and mass ratios.

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