Rotational mode splitting about an inclined axis

Details Rotational mode splitting about an inclined axis Rotational mode splitting about an inclined axis

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...286l..43a&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 286, Nov. 15, 1984, p. L43-L45.

Astronomy and Astrophysics

Astrophysics

8

Stellar Oscillations, Stellar Rotation, Variable Stars, Angular Velocity, Cartesian Coordinates, Integral Equations, Spherical Harmonics

Scientific paper

The authors have derived the "m-splitting" formula for the frequencies of nonradial oscillations of stars due to slow rotation about an axis which is inclined with respect to the pulsation axis. They obtain the simple result that the usual formula applies, except that only the component of the angular rotation velocity along the pulsation axis, rather than the full angular rotation velocity, is to be used in this formula.

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