Perturbations in close binary systems produced by the tides lagging in latitude

Details Perturbations in close binary systems produced by the tides lagging in latitude Perturbations in close binary systems produced by the tides lagging in latitude

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.137..139z&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 137, no. 1, Oct. 1987, p. 139-149.

Astronomy and Astrophysics

Astrophysics

Binary Stars, Orbit Perturbation, Periodic Variations, Secular Variations, Tides, Latitude, Nonlinear Equations, Orbital Elements

Scientific paper

The aim of this investigation is to present the periodic and secular perturbations of the orbital elements of close binary systems due to tidal lag in latitude. The variational equations of the problem of plane motion are set up in terms of the rectangular components R, S, and W of the disturbing accelerations. These equations are highly nonlinear with respect to the orbital elements and the author presents analytic approximations to the effects produced by the perturbing acceleration due to dynamical tides lagging in latitude. The perturbed elements of the orbit have been expressed by means of Hansen coefficients in the compact form of summations.

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