The Influence of Rotation on the Pulsation Spectra of B-stars

Details The Influence of Rotation on the Pulsation Spectra of B-stars The Influence of Rotation on the Pulsation Spectra of B-stars

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011spd....42.1619m&link_type=abstract

American Astronomical Society, SPD meeting #42, #16.19; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

B stars are known to oscillate in both radial and non-radial modes. Rotation may play an important role in altering the pulsation spectra of these stars. The results of 2D model calculations of rapidly rotating early B-stars is presented and used to examine the frequency spectrum of a Kepler B-star. The reduction procedure to determine stellar pulsation spectra using Kepler data sets is discussed, as well as the need for additional observational data to constrain the B-star spherical harmonic l and m values. This work is supported by the NASA Kepler Guest Observer program.

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