Elliptical rings in binary systems

Details Elliptical rings in binary systems Elliptical rings in binary systems

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.207..215w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 207, March 1, 1984, p. 215-222.

Statistics

Computation

7

Binary Stars, Ring Structures, Stellar Mass Accretion, Stellar Structure, Variable Stars, Computerized Simulation, Stellar Models

Scientific paper

One explanation of the currently known properties of SU UMa stars in supermaximum includes the formation of an elliptical accretion ring. The results of numerical computations of stream flow in binary systems are presented. It is pointed out that the previous interpretation of these trajectories is erroneous and that elliptical rings cannot survive longer than a few orbits in the primary's Roche lobe following a mass transfer event through the inner Lagrangian point.

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