EVOLUTIONARY TRACKS of 1.6 to 20 M_Sun stellar models with new OP opacities

J. Daszyńska-Daszkiewicz, P. Walczak, 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 A04 (Asplund et al. 2005).

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• X = 0.65, Z = 0.020, V = 0 (a04)
• X = 0.70, Z = 0.010, V = 0 (a04)
• X = 0.70, Z = 0.015, V = 0 (a04)
• X = 0.70, Z = 0.020, V = 0 (a04)
• X = 0.70, Z = 0.020, V = 200 (a04)
• X = 0.75, Z = 0.020, V = 0 (a04)
• X = 0.70, Z = 0.030, V = 0 (a04)
• X = 0.70, Z = 0.020, V = 50 (a04)
• X = 0.70, Z = 0.020, V = 100 (a04)
• X = 0.70, Z = 0.015, V = 50 (a04)
• X = 0.70, Z = 0.015, V = 100 (a04)
• X = 0.70, Z = 0.015, V = 200 (a04)
• X = 0.65, Z = 0.015, V = 0 (a04)
• X = 0.70, Z = 0.015, V = 50 (a04)
• X = 0.70, Z = 0.009, V = 0 (a04)
• X = 0.70, Z = 0.02, V = 50 (a04)

REFERENCES:

• Asplund M., Grevesse N., Sauval A.J., 2004, ASP Conf. Ser, 336, 25