Gas stream characteristics in the vicinity of the inner Lagrangian point in R CMa stars.

Details Gas stream characteristics in the vicinity of the inner Lagrangian point in R CMa stars. Gas stream characteristics in the vicinity of the inner Lagrangian point in R CMa stars.

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996kpcb...12...35k&link_type=abstract

Kinematics Phys. Celest. Bodies, Vol. 12, No. 4, p. 35 - 38

Physics

Semi-Detached Systems: Gas Motions, Semi-Detached Systems: Hydrodynamics

Scientific paper

Gas stream structure in the vicinity of the inner Lagrangian point was calculated for four R CMa-type eclipsing binaries using the Euler hydrodynamics equations and the big-particles method of Belotserkovskii and Davydov. The stream characteristics are found to be different for stars with mass ratios less than 0.1 and more than 0.1; the mass transfer is quasi-conservative.

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