Evolutionnary models for solar twins (do Nascimento+, 2009)

Details Evolutionnary models for solar twins (do Nascimento+, 2009) Evolutionnary models for solar twins (do Nascimento+, 2009)

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..35010687d&link_type=abstract

VizieR On-line Data Catalog: J/A+A/501/687. Originally published in: 2009A&A...501..687D

Physics

Abundances, Hr Diagrams, Models: Evolutionary, Stars: Ages, Stars: Masses

Scientific paper

The models are computed by using the Toulouse-Geneva stellar evolution code TGEC (Hui-Bon-Hoa, 2008, Ap&SS, 316, 55). Details of the physics of these models can be found in Richard et al. (1996A&A...312.1000R, 2004, SoPh, 220, 243), do Nascimento et al. (2000A&A...357..931D), and Hui-Bon-Hoa (2008, Ap&SS, 316, 55). We computed evolutionary models of different masses from the zero-age main sequence (ZAMS) to the end of the hydrogen exhaustion in the core. The calibration method of the models is based on the Richard et al. (1996A&A...312.1000R) prescription.
(3 data files).

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