The influence of viscosity on tidal flows in binary stellar systems.
Abstract
Solutions to hydrodynamic equations are used to obtain explicit analytical expressions for tidal flow velocities in the component of a binary system with allowance for viscosity. Allowance is made for stellar rotation, the orbit eccentricity, and the inclination of the axis of rotation to the orbital plane. Velocities are calculated for different star systems.
 Publication:

Pisma v Astronomicheskii Zhurnal
 Pub Date:
 July 1989
 Bibcode:
 1989PAZh...15..625D
 Keywords:

 Binary Stars;
 Computational Astrophysics;
 Stellar Systems;
 Tides;
 Viscosity;
 Energy Dissipation;
 Flow Velocity;
 Hydrodynamic Equations;
 Stellar Orbits;
 Stellar Rotation;
 Astrophysics