Preliminary results of the effects of fast shellular rotation on the oscillation spectrum of delta-Scuti stars

Details Preliminary results of the effects of fast shellular rotation on the oscillation spectrum of delta-Scuti stars Preliminary results of the effects of fast shellular rotation on the oscillation spectrum of delta-Scuti stars

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..227s&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

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The rotation treatment has been improved during the last decades for seismological studies. An oscillation code following Soufi et al, 1998 which takes into account the structure deformation of the star due to the centrifugal force. In the present work we revisit the interesting case of GX Pegasi from which we have quite wide seismological information (Goupil et al, 1992). We propose a preliminary study of the oscillations frequencies for GX Pegasi, using the technics mentioned above.

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