Computer simulations of gas flow around close binary systems

Details Computer simulations of gas flow around close binary systems Computer simulations of gas flow around close binary systems

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..33..465s&link_type=abstract

Astrophysics and Space Science, vol. 33, Apr. 1975, p. 465-480.

Astronomy and Astrophysics

Astrophysics

20

Binary Stars, Computerized Simulation, Density Distribution, Gas Flow, Velocity Distribution, Astronomical Models, Mass Flow, Ring Structures, Roche Limit, Time Dependence

Scientific paper

A gas-dynamical model of gas streams around close binary systems is given. The velocity field and the density distribution are determined for different parameter ranges. The results succeed in explaining the formation of a ring and a disk around the accreting component. The models furthermore reveal the existence of a tongue of matter extending from the inner Lagrangian point and a jet perpendicular to the system axis.

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