Looking into B star interiors by means of asteroseismology

Computer Science – Databases

Scientific paper

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Normal Stars : General Or Individual, Astronomical Observations, Pulsars, Origin And Formation Of The Universe, Stellar Clusters And Associations, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc., Astronomical And Space-Research Instrumentation

Scientific paper

Precise modeling of upper main sequence stars is important in various astrophysical contexts, including chemical evolution of the Universe. However, there are still significant uncertainties resulting mostly, but not only, from our poor understanding of transport processes. Data on pulsating objects, in particular β Cephei stars, provide us valuable constraints on parameters describing efficiency of these processes and asses the overall accuracy of present stellar models. I review methods of extracting information on stellar interior structure and rotation from pulsation data and present some recent results for selected objects.

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