Physics
Scientific paper
Oct 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jphcs.118a2021e&link_type=abstract
Journal of Physics: Conference Series, Volume 118, Issue 1, pp. 012021 (2008).
Physics
Scientific paper
The computation of models of stars for which solar-like oscillations have been observed is discussed. After a brief intoduction on the observations of solar-like oscillations, the modelling of isolated stars and of stars belonging to a binary system is presented with specific examples of recent theoretical calibrations. Finally the input physics introduced in stellar evolution codes for the computation of solar-type stars is discussed with a peculiar emphasis on the modelling of rotation for these stars.
Carrier Fabien
Eggenberger Patrick
Mathis Stephane
Miglio Andrea
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