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.Comment: Invited review paper to appear in Proc. IAU307: New windows on
massive stars: asteroseismology, interferometry, and spectropolarimetry,
Editors: G. Meynet, C. Georgy, J.H. Groh & Ph. Stee, 9 pages, 2 figure
