We present a project aimed at self-consistently deriving the physical parameters and chemical composition of massive pulsators (β Cephei stars, Slowly Pulsating B stars) based on high-resolution optical spectra. Such data will be essential for a proper theoretical interpretation of their oscillation spectrum, but may also contribute in a broader context to our understanding of mixing and diffusion processes in B-type stars. As an illustration, our first results reveal the existence of core-processed material at the surface of some slowly-rotating β Cephei stars which is not predicted by current evolutionary models including rotation.
CITATION STYLE
Morel, T., Briquet, M., & Aerts, C. (2008). Precision Spectroscopy in Astrophysics. (N. C. Santos, L. Pasquini, A. C. M. Correia, & M. Romaniello, Eds.), Precision Spectroscopy in Astrophysics (pp. 301–302). Springer Berlin Heidelberg. Retrieved from http://adsabs.harvard.edu/abs/2008psa..conf..301M
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