Evolution and Pulsations of Massive Stars on the Main Sequence and Close to it
7-11 July, 2008
Venue: Liège (Belgium)
The main idea of this colloquium is first to close in on the problems raised by "non standard" physics, second, to focus on the effects of these often missing physical processes on stellar evolution and third, to analyse what asteroseismology can do to bring a new light on these processes and their modelling. The targets are massive stars (O, B, WR) for which new and exciting results are now coming from asteroseismic interpretations of observed modes.