Non-radial pulsations and stability of massive stars

Details Non-radial pulsations and stability of massive stars Non-radial pulsations and stability of massive stars

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.282.1470g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 282, Issue 4, pp. 1470-1482.

Other

24

Instabilities, Stars: Oscillations, Stars: Variables: Other

Scientific paper

A non-radial non-adiabatic linear stability analysis of stellar models with initial masses on the zero-age main sequence (ZAMS) between 20 and 80 M_solar is presented. Two groups of dynamical mode-coupling instabilities are identified. We examine the influence of the treatment of convection on these instabilities, as well as their dependence on the stellar mass and the harmonic degree l of the perturbation. The instabilities are discussed within the context of a recently proposed model for strange-mode instabilities.

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