Numerical simulations in cosmic gas dynamics: Gas flows in binary stars

Details Numerical simulations in cosmic gas dynamics: Gas flows in binary stars Numerical simulations in cosmic gas dynamics: Gas flows in binary stars

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985tmsf.proc...51m&link_type=abstract

In Tokyo Univ. Proceedings of the Symposium on Mechanics for Space Flight p 51-66 (SEE N86-23858 14-34)

Statistics

Computation

Binary Stars, Computation, Gas Dynamics, Gas Flow, Simulation, Stellar Mass Ejection, Stellar Winds, Classifications, Finite Difference Theory, Shock Waves, X Rays

Scientific paper

Examples of numerical simulation in cosmic gasdynamics, i.e. gas flows in close binary stars, are presented. The first example is a calculation of Roche lobe overflow in a semidetached binary system. The second one is an interaction of stellar wind blowing from the mass losing star with another star. The third example is a mass loss from a contact binary system. Finite difference schemes are used to calculate gas flows. In either cases shock waves are formed because of gravitational focusing effect.

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