Another look at the r-modes

Details Another look at the r-modes Another look at the r-modes

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.135..393k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 135, no. 2, July 1987, p. 393-398.

Statistics

Computation

Hydrodynamic Equations, Stellar Oscillations, Stellar Rotation, Vibration Mode, Angular Velocity, Computational Fluid Dynamics, Mass Transfer, Spherical Coordinates

Scientific paper

Possible oscillation modes for a rotating star are listed. The only
assumption made is that oscillations are adiabatic and that rotation is
uniform. It is found that two modes not present for non-rotating stars
are possible. Oscillation frequencies of these modes are rather
different from those given in the literature for so-called r-modes.

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