Isochrones for an Extended Region of the Z-Y Plane Including New Asymptotic Giant Branch Models

Details Isochrones for an Extended Region of the Z-Y Plane Including New Asymptotic Giant Branch Models Isochrones for an Extended Region of the Z-Y Plane Including New Asymptotic Giant Branch Models

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..374...41b&link_type=abstract

From Stars to Galaxies: Building the Pieces to Build Up the Universe. ASP Conference Series, Vol. 374, proceedings of the confer

Statistics

Computation

Scientific paper

A large project for the computation of stellar tracks and isochrones covering an extended region of the Z-Y plane has been undertaken to allow people to model stellar populations for different helium enrichment values. TP-AGB computations are included with variable molecular opacities adopting low-temperature opacities properly evaluated for the chemical mixtures of evolving TP-AGB models, instead of usual scaled-solar ones. We evaluate the effects of a significant helium enhancement on bolometric corrections and T_{eff}-colour relations.

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