Ścieżki ewolucyjne dla gwiazd o masach od 1.8 do 12.0 Msun wyznaczone przy użyciu nieprzeźroczystości OPAL

J. Daszyńska-Daszkiewicz, Instytut Astronomiczny Uniwersytetu Wrocławskiego

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).

Pobierz:

• X = 0.70, Z = 0.020

BIBLIOGRAFIA:

• 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