Forced oscillations in binary systems - Toroidal modes

Details Forced oscillations in binary systems - Toroidal modes Forced oscillations in binary systems - Toroidal modes

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...111..252r&link_type=abstract

Astronomy and Astrophysics, vol. 111, no. 2, July 1982, p. 252-254.

Astronomy and Astrophysics

Astrophysics

9

Binary Stars, Forced Vibration, Stellar Gravitation, Stellar Oscillations, Stellar Rotation, Eccentric Orbits, Eigenvalues, Stellar Models

Scientific paper

The forced oscillations of a star, due to a periodic varying outer gravitational potential are examined, more precisely concerning toroidal modes. The oscillations are assumed to be adiabatic and the star uniformly and slowly rotating. The results show that for most of these modes, a resonance is possible only for determined values of the ratio of the orbital to rotation frequency. The importance of this resonance is comparable to those of gravity modes, for sufficiently large values of the stellar rotation.

Affiliated with

Also associated with

No associations

Rating

Forced oscillations in binary systems - Toroidal modes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Forced oscillations in binary systems - Toroidal modes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Forced oscillations in binary systems - Toroidal modes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1022072