Tides in asynchronous binary systems

@inproceedings{Toledano2006TidesIA,
  title={Tides in asynchronous binary systems},
  author={Ohad Toledano and Edmundo Vergara Moreno and Gloria Koenigsberger and R. G. Detmers and Norbert Langer},
  year={2006}
}
Stellar oscillations are excited in non-synchronously rot ating stars in binary systems due to the tidal forces. Tangential components of the tides can drive a shear flow whic h behaves as a di fferentially forced rotating structure in a stratified outer medium.