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Massive Star Asteroseismology in Action

Published online by Cambridge University Press:  23 January 2015

Conny Aerts
Conny Aerts*
Affiliation:
Institute of Astronomy, KU Leuven, Celestijnenlaan 200 D, 3001 Leuven, Belgium email: [email protected] Department of Astrophysics/IMAPP, Radboud University Nijmegen, 6500 GL Nijmegen, the Netherlands
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Abstract

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After highlighting the principle and power of asteroseismology for stellar physics, we briefly emphasize some recent progress in this research for various types of stars. We give an overview of high-precision high duty-cycle space photometry of OB-type stars. Further, we update the overview of seismic estimates of stellar parameters of OB dwarfs, with specific emphasis on convective core overshoot. We discuss connections between pulsational, rotational, and magnetic variability of massive stars and end with future prospects for asteroseismology of evolved OB stars.

Keywords

asteroseismologystars: oscillations (including pulsations)stars: interiorsstars: evolutionstars: rotationmethods: data analysismethods: statisticalmagnetic fieldswavesturbulence
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Issue S307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry , June 2014 , pp. 154 - 164
Copyright
Copyright © International Astronomical Union 2015 

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