Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982afz....18..151s&link_type=abstract
(Astrofizika, vol. 18, Jan.-Mar. 1982, p. 151-160.) Astrophysics, vol. 18, no. 1, July 1982, p. 90-96. Translation.
Astronomy and Astrophysics
Astrophysics
Binary Stars, Companion Stars, Stellar Oscillations, Stellar Rotation, Adiabatic Conditions, Equations Of Motion, Homogeneity, Radial Velocity
Scientific paper
The equation of small adiabatic radial pulsations of a star rotating as a rigid body is derived. This equation is used in the special case of a homogeneous star. The perturbations of order Omega-squared are taken into account and all radial modes are considered. It is shown that the frequencies of the radial pulsations of the rotating star are less than the corresponding frequencies of a nonrotating star of the same mass. The ratios of the periods of the overtones change very little. Tidal forces do not change the frequencies of the radial pulsations.
No associations
LandOfFree
Influence of rotation and a binary companion on the frequency of the radial pulsations of a homogeneous star 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 Influence of rotation and a binary companion on the frequency of the radial pulsations of a homogeneous star, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Influence of rotation and a binary companion on the frequency of the radial pulsations of a homogeneous star will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1455194