Space oscillations of stellar non radial eigen-functions

Details Space oscillations of stellar non radial eigen-functions Space oscillations of stellar non radial eigen-functions

Sep 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974a%26a....34..449s&link_type=abstract

Astronomy and Astrophysics, vol. 34, no. 3, Sept. 1974, p. 449-451.

Astronomy and Astrophysics

Astrophysics

6

Astronomical Models, Stellar Structure, Vibration Mode, Eigenvectors, Perturbation Theory, Pressure Effects, Spherical Harmonics, Stellar Evolution

Scientific paper

It is generally believed that the g(minus) modes of nonradial oscillations of a star may oscillate only in convective zones, and that the g(plus) modes may oscillate only in radiative zones. Whereas the first statement may be proved quite generally, the second one is true only in the inner part of the star. With this restriction it is valid also for p modes.

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