000002822 001__ 2822
000002822 005__ 20160701171711.0
000002822 0247_ $$2DOI$$a10.1017/S1743921311011070
000002822 037__ $$aASTROimport-979
000002822 100__ $$aDe Cat, P.
000002822 245__ $$aAsteroseismic observations of OB stars
000002822 260__ $$c2011
000002822 520__ $$aThe region of the hot end of the main-sequence is hosting pulsating stars of different types and flavours. Pulsations are not only observed for Slowly pulsating B stars (mid to late B-type stars; high order g-modes) and ß Cephei stars (early B-type stars; low order p/g-modes) but are also causing variability in Be stars and OB-supergiants. In this review we give an overview of the asteroseismic observations that are currently available for these types of stars. The first asteroseismic results were solely based on ground-based observations. Recently, the arrival of space-based data gathered by space missions like most, corot and kepler has led to important discoveries for massive stars, highlighting their excellent asteroseismic potential. We show that, despite the unprecedented precision of the space-based data, there is still a clear need for ground-based follow-up observations. 
000002822 700__ $$a Uytterhoeven, K.
000002822 700__ $$a Gutiérrez-Soto, J.
000002822 700__ $$a Degroote, P.
000002822 700__ $$a Simón-Díaz, S.
000002822 773__ $$c433-444$$pActive OB Stars: Structure, Evolution, Mass Loss, and Critical Limits$$v272$$y2011
000002822 85642 $$ahttp://esoads.eso.org/abs/2011IAUS..272..433D
000002822 905__ $$apublished in
000002822 980__ $$aNONREF