Equipotential surfaces in close binary systems - Remarks on the time-dependent potential function

Details Equipotential surfaces in close binary systems - Remarks on the time-dependent potential function Equipotential surfaces in close binary systems - Remarks on the time-dependent potential function

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.187..119t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 187, Jan. 1992, p. 119-126.

Astronomy and Astrophysics

Astrophysics

Binary Stars, Equipotentials, Gravitational Fields, Stellar Gravitation, Stellar Rotation, Time Dependence, Angular Velocity, Celestial Mechanics, Equations Of Motion, Kepler Laws

Scientific paper

By use of the mass-point model, the equations of the equipotential
surfaces are reviewed. A difference between the time-dependent potential
function and zero relative velocity surfaces is put in evidence. A
drawback in the time-dependent transformation between the (xi, eta,
zeta) and (x, y, z) coordinate systems is underlined.

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