The asymptotic representation of dynamic tides in close binaries revisited

Details The asymptotic representation of dynamic tides in close binaries revisited The asymptotic representation of dynamic tides in close binaries revisited

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...336..539s&link_type=abstract

Astronomy and Astrophysics, v.336, p.539-544 (1998)

Astronomy and Astrophysics

Astrophysics

1

Stars: Binaries: Close, Methods: Analytical, Celestial Mechanics, Stellar Dynamics

Scientific paper

The asymptotic representation of low-frequency, linear, isentropic dynamic tides in components of close binaries derived by Smeyers (1997) is reconsidered. The constructions of the second-order boundary-layer solutions for the divergence and the radial component of the tidal displacement are made more transparent. Moreover, the determination of the constants involved in the second-order boundary-layer solution for the radial component of the tidal displacement valid near the star's surface is modified. As a result, a corrected expression for the second-order Eulerian perturbation of the gravitational potential at the star's surface caused by the tidal distortion is obtained.

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