Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.213..279c&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 213, March 15, 1985, p. 279-293.
Astronomy and Astrophysics
Astronomy
6
Binary Stars, Blue Stars, Celestial Mechanics, Radio Sources (Astronomy), Stellar Motions, Doppler Effect, Line Spectra, Plasma Jets, Precession, Stellar Models, Stellar Oscillations, Tides, Variable Stars
Scientific paper
A dynamical formalism for describing the motion of a distorted object moving under the influence of the gravitational fields present in a close binary system is developed. The object is assumed to be centered about one of the components and to have a form or shape sustained by axial forces such as rotation in addition to tides generated by the companion. Although such a shape will not be temporally constant, the moments of inertia are expressible in terms of the canonical coordinates of the problem and vary in a periodic manner. The dynamical behavior of this 'elastic' body can be expressed in terms of periodic motion analogous to that found in a rigid body. The details of the resultant motion in turn places constraints on the nature of the components of the system.
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