Tidal flows in binary systems with noncircular orbits

Details Tidal flows in binary systems with noncircular orbits Tidal flows in binary systems with noncircular orbits

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..301d&link_type=abstract

(Astronomicheskii Zhurnal, vol. 62, Mar.-Apr. 1985, p. 301-305) Soviet Astronomy (ISSN 0038-5301), vol. 29, Mar.-Apr. 1985, p. 1

Astronomy and Astrophysics

Astronomy

6

Binary Stars, Eccentric Orbits, Stellar Orbits, Tides, Angular Velocity, Spherical Harmonics, White Dwarf Stars

Scientific paper

Expressions are derived for the velocities of tidal flows in close binary star systems with eccentric orbits. The third spherical harmonic is taken into account in the expansion of the tidal-interaction expansion. The solutions are applicable to the giant planets of the solar system and to white dwarfs without the introduction of corrections for compressibility. The Saturn-Titan system and the binary system BD + 16 deg 516 (V 471 Tau) are considered as examples.

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