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What physics is missing in theoretical models of high-mass stars: new insights from asteroseismology

Asteroseismology of massive stars has recently begun a revolution thanks to high-precision time series photometry from space telescopes. This has allowed accurate and robust constraints on interior physical processes, such as mixing and rotation in the near-core region of stars, to be determined across different masses and ages. In this review, I discuss recent advances in our knowledge of massive star interiors made by means of gravity-mode asteroseismology, and highlight some new observational discoveries of variability in some of the most massive stars in our universe.

preprint2019arXivOpen access
D. M. Bowman
astro-ph.SR
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D. M. Bowman

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