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- W2996801438 abstract "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." @default.
- W2996801438 created "2020-01-10" @default.
- W2996801438 creator A5003101576 @default.
- W2996801438 date "2019-12-29" @default.
- W2996801438 modified "2023-09-25" @default.
- W2996801438 title "What physics is missing in theoretical models of high-mass stars: new insights from asteroseismology" @default.
- W2996801438 doi "https://doi.org/10.48550/arxiv.1912.12653" @default.
- W2996801438 hasPublicationYear "2019" @default.
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