EVOLUTIONARY TRACKS of 1.8 to 12.0 Msun stellar models with OPAL opacities

J. Daszyńska-Daszkiewicz, Astronomical Institute, University of Wrocław

The evolutionary tracks have been calculated for stellar models from 1.8 up to 12 solar masses in the MS and early post-MS evolutionary stages. The results were obtained for Z=0.020 and reffered as GN93 (Grevesse & Noels 1993).

Download:

• X = 0.70, Z = 0.020

REFERENCES:

• Grevesse N., Noels A., 1993, in Pratzo M., Vangioni-Flam E., Casse M., eds., Origin and Evolution of the Elements, Cambridge Univ. Press, p. 15