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Asteroseismology of massive stars has recently begun a revolution thanks tohigh-precision time series photometry from space telescopes. This has allowedaccurate and robust constraints on interior physical processes, such as mixingand rotation in the near-core region of stars, to be determined acrossdifferent masses and ages. In this review, I discuss recent advances in ourknowledge of massive star interiors made by means of gravity-modeasteroseismology, and highlight some new observational discoveries ofvariability in some of the most massive stars in our universe.

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