Year: 2006
Type: article
Abstract: Context.Stellar oscillations are excited in non-synchronously rotating stars in binary systems due to the tidal forces. Tangential components of the tides can drive a shear flow which behaves as a differentially forced rotating structure in a stratified outer medium.
Source: Astronomy and Astrophysics
Authors: O. Toledano, E. Moreno, G. Koenigsberger, R. Detmers, N. Langer
Institutions: Universidad Nacional Autónoma de México, Utrecht University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W2165541763
