Accurate integrations of the Roche model

Details Accurate integrations of the Roche model Accurate integrations of the Roche model

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apjs...55..551m&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 55, Aug. 1984, p. 551-561.

Astronomy and Astrophysics

Astrophysics

69

Binary Stars, Roche Limit, Stellar Models, Astrometry, Astronomical Catalogs, Cartesian Coordinates, Mass Ratios, Stellar Mass, Stellar Rotation

Scientific paper

The Roche model for close binary systems in synchronous rotation is accurately integrated to give volume radii, surface areas, mean gravities, and mean inverse gravities in normalized units. The range of fill-out is 0.2 ≤ F ≤ 2.0, and for smaller fill-out factors a simple analytical approximation is adequate. The mass ratio range is 0.04 ≤ q ≤ 1.0. A table of contact potentials is given for 0.01 ≤ q ≤ 1.0.

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