Tidal resonances in binary star systems. II - Slowly rotating stars

Details Tidal resonances in binary star systems. II - Slowly rotating stars Tidal resonances in binary star systems. II - Slowly rotating stars

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.235.1367a&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 235, Dec. 15, 1988, p. 1367-1383.

Astronomy and Astrophysics

Astronomy

3

Binary Stars, Orbital Resonances (Celestial Mechanics), Stellar Rotation, Eccentricity, Hamiltonian Functions, Kepler Laws, Stellar Oscillations, Tides

Scientific paper

The potential energy of tidal interactions in a binary system with rotating components is formulated as a perturbation Hamiltonian which self-consistently couples the dynamics of the rotating stars' oscillations and orbital motion. The action-angle formalism used to discuss tidal resonances in the nonrotating case (Alexander, 1987) is extended to rotating stars. The behavior of a two-mode system and the procedure for treating an arbitrary number of modes are discussed.

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