WROCŁAW HELAS WEBPAGE

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

J. Daszyńska-Daszkiewicz, P. Walczak, Astronomical Institute, University of Wroc³aw

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