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The effect of turbulent mixing on the g-mode spectrum of MS stars
J. Montalban, A. Miglio, P. Eggenberger +1
The understanding of transport processes inside the stars is one of the main goals of asteroseismology. Chemical turbulent mixing can affect the internal distribution of μnear the…
Gravity modes and mixed modes as probes of stellar cores in main-sequence stars: from solar-like to beta Cep stars
A. Miglio, J. Montalban, P. Eggenberger +1
We investigate how the frequencies of gravity modes depend on the detailed properties of the chemical composition gradient that develops near the core of main-sequence stars and, t…
The Liege Oscillation Code
R. Scuflaire, J. Montalban, S. Theado +5
The Liege Oscillation code can be used as a stand-alone program or as a library of subroutines that the user calls from a Fortran main program of his own to compute radial and non-…
CLES, Code Liegeois d'Evolution Stellaire
R. Scuflaire, S. Theado, J. Montalban +5
Cles is an evolution code recently developed to produce stellar models meeting the specific requirements of studies in asteroseismology. It offers the users a lot of choices in the…
Inter-comparison of the g-, f- and p-modes calculated using different oscillation codes for a given stellar model
A. Moya, J. Christensen-Dalsgaard, S. Charpinet +9
In order to make astroseismology a powerful tool to explore stellar interiors, different numerical codes should give the same oscillation frequencies for the same input physics. Th…
Close-up of primary and secondary asteroseismic CoRoT targets and the ground-based follow-up observations
K. Uytterhoeven, E. Poretti, M. Rainer +13
To optimise the science results of the asteroseismic part of the CoRoT satellite mission a complementary simultaneous ground-based observational campaign is organised for selected…