TL;DR
This paper reviews recent advances in asteroseismology of massive stars, highlighting space photometry, stellar parameter estimation, and the interplay of pulsation, rotation, and magnetic fields, with future outlooks.
Contribution
It provides a comprehensive overview of recent progress and future prospects in asteroseismology of OB-type stars, emphasizing high-precision space photometry and stellar parameter estimation.
Findings
High-precision space photometry enables detailed stellar analysis.
Seismic methods improve estimates of stellar parameters like core overshoot.
Connections between pulsational, rotational, and magnetic variability are explored.
Abstract
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.
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