Self-Consistent Stellar Evolution Models with Updated Physics and Variable Abundances

Details Self-Consistent Stellar Evolution Models with Updated Physics and Variable Abundances Self-Consistent Stellar Evolution Models with Updated Physics and Variable Abundances

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...209.4003d&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #40.03; Bulletin of the American Astronomical Society, V

Physics

2

Scientific paper

Results from stellar evolution calculations using updated input physics, a detailed equation of state, and model atmosphere boundary conditions in a state of the art stellar evolution code are presented. The stellar evolution models cover evolutionary phases from the pre-main sequence to the onset of thermal pulsations on the asymptotic giant branch. The results are applied to study a variety of topics including: globular cluster age determinations using the data from the HST-ACS Galactic Globular Cluster Survey, the effects of separately enhancing individual elements on the morphology of isochrones in the H-R diagram, very low mass stars in NGC 6397, and stellar population models.

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