Physics
Scientific paper
Nov 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coast.156...91g&link_type=abstract
Communications in Asteroseismology, Vol.156, p. 91-92
Physics
Scientific paper
The main idea of this colloquium was first, to close in on the problems raised by "nonstandard" physics, second, to focus on the effects of these often missing physical processes on stellar evolution and third, to analyze what asteroseismology could do to shed a new light on these processes and their modeling. The targets are massive stars (O, B, WR) for which new and exciting results are now coming from asteroseismic interpretations of observed modes.
The main objectives were threefold. In a first part, physical processes involved in "nonstandard" modeling such as semiconvection, overshooting and convective penetration, rotation, diffusion,... were analyzed in detail. A second part focused on the problems related to the effect of such "nonstandard" processes on stellar modeling. The third part introduced asteroseismology as a probe of the internal structure of stars, in particular in the frame of present and future asteroseismology missions, from space or ground-based, such as CoRoT, KEPLER, PLATO, SIAMOIS, SONG,...
In what follows, we present a flavor of the topics discussed in seven sessions covering these three parts.
Grötsch-Noels A.
Miglio Andrea
Montalban Josefina
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