Scientific rationale
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.

7 January 2008 Conference registration opens
29 February 2008 Request financial support deadline
30 April 2008 Abstract submission deadline
30 April 2008 Conference registration closes
15 May 2008 Selection of contributed talks
7 July 2008 Conference starts!