Scaled solar tracks and isochrones (Bertelli+, 2008)

Details Scaled solar tracks and isochrones (Bertelli+, 2008) Scaled solar tracks and isochrones (Bertelli+, 2008)

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34840815b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/484/815. Originally published in: 2008A&A...484..815B

Astronomy and Astrophysics

Astrophysics

Models: Evolutionary

Scientific paper

In many astrophysical contexts, the helium content of stars may differ significantly from those usually assumed in evolutionary calculations.
In order to improve upon this situation, we have computed tracks and isochrones in the range of initial masses 0.15-20M{sun} for a grid of 39 chemical compositions with the metal content Z between 0.0001 and 0.070 and helium content Y between 0.23 and 0.46.
************************************************************************** * * * Sorry, but the author(s) never supplied the tabular material * * announced in the paper * * * **************************************************************************

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