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Asteroseismology of binary stars and a compilation of core overshoot and rotational frequency values of OB stars

Published online by Cambridge University Press:  25 February 2014

C. Aerts
C. Aerts*
Affiliation:
Institute of Astronomy, KU Leuven, 3001 Leuven, Belgium Department of Astrophysics, IMAPP, Radboud University Nijmegen, The Netherlands
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Abstract

After a brief introduction into the asteroseismic modelling of stars, we provide a compilation of the current seismic estimates of the core overshooting parameter and of the rotational frequency of single and binary massive stars. These important stellar parameters have meanwhile become available for eleven OB-type stars, among which three spectroscopic pulsating binaries and one magnetic pulsator. We highlight the potential of ongoing and future analyses of eclipsing binary pulsators as essential laboraties to test stellar structure and evolution models of single and binary stars.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 64: Setting a New Standard in the Analysis of Binary Stars , 2013 , pp. 323 - 330
Copyright
© EAS, EDP Sciences, 2014

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