Matter stream formation in close binaries

Details Matter stream formation in close binaries Matter stream formation in close binaries

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997kfnt...13b..39n&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 13, p. 39

Physics

Binary Stars, Matter (Physics), Hydrodynamic Equations, Eccentric Orbits, Coriolis Effect, Stellar Orbits, Analytic Functions

Scientific paper

The dependence of the matter stream structure on the Coriolis force and
the overflow degree has been calculated using numerical hydrodynamical
methods. A comparison is made with analytical dependences. Using these
calculations, the possible mass transfer rate variations due to
eccentricity of the orbital motion are determined.

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