On the tidal interaction of a solar-type star with an orbiting companion: Excitation of g mode oscillation and orbital evolution

We calculate the dynamical tides raised on a non-rotating solar-type star by a close stellar or planetary companion. Dissipation arising from a turbulent viscosity operating in the convection zone and radiative damping in the radiative core are considered. We compute the torque exerted on the star b...

Täydet tiedot

Bibliografiset tiedot
Päätekijät: Terquem, C, Papaloizou, J, Nelson, R, Lin, D
Aineistotyyppi: Journal article
Kieli:English
Julkaistu: Institute of Physics Publishing 1998