Stellar Evolution and Seismic Tools for Asteroseismology - Diffusive Processes in Stars and Seismic Analysis
C.W. Straka, Y. Lebreton and M.J.P.F.G. Monteiro (eds)
EAS Publications Series, 26 (2007) 177-185
DOI: 10.1051/eas:2007136
Comparisons for ESTA-Task3: ASTEC, CESAM and CLÉS
J. Christensen-DalsgaardDanish AsteroSeismology Centre, and Department of Physics and Astronomy, University of Aarhus, 8000 Aarhus C, Denmark
(Published online: 20 June 2007)
Abstract
The ESTA activity under the CoRoT project aims at testing the tools for
computing stellar models and oscillation frequencies that will be used
in the analysis of asteroseismic data from CoRoT and other large-scale
upcoming asteroseismic projects.
Here I report results of comparisons between calculations using
the Aarhus code (ASTEC) and two other codes, for models that include
diffusion and settling.
It is found that there are likely deficiencies, requiring further study,
in the ASTEC computation of models including convective cores.
© EAS, EDP Sciences 2007


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