The CoRoT and Kepler data revolutionised our view on stellar pulsation. For
massive stars, the space data revealed the simultaneous presence of
low-amplitude low-order modes and dominant high-order gravity modes in several
B-type pulsators. The interpretation of such a rich set of detected
oscillations requires new tools. We present computations of oscillations for
B-type pulsators taking into account the effects of the Coriolis force in the
so-called traditional approximation. We discuss the limitations of classical
frequency matching to tune these stars seismically and show that the predictive
power is limited in the case of high-order gravity mode pulsators, except if
numerous modes of consecutive radial order can be identified.Comment: 8 pages, 4 figures. Paper submitted for publication in the
Proceedings of the 61st Fujihara Seminar: Progress in solar/stellar physics
with helio- and asteroseismology to appear in ASP Conference Serie
