The non-radial stability of Wolf-Rayet stars

Details The non-radial stability of Wolf-Rayet stars The non-radial stability of Wolf-Rayet stars

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mnras.337..743g&link_type=abstract

Monthly Notice of the Royal Astronomical Society, Volume 337, Issue 2, pp. 743-748.

Other

8

Instabilities, Stars: Oscillations, Stars: Variables: Other, Stars: Wolf-Rayet

Scientific paper

A non-radial non-adiabatic linear stability analysis of selected models for Wolf-Rayet stars is presented. Strange-mode instabilities with growth rates in the dynamical range are found to affect both radial and non-radial perturbations up to the harmonic degree l~ 250. On the basis of the results of the non-radial stability analysis it is argued that strange modes and associated instabilities are caused by mode pairing of ordinary acoustic modes. Some implications of the non-radial instability of Wolf-Rayet stars are discussed.

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