All computations were performed using Warsaw-New Jersey evolutionary
code of Paczyński. For description of the code see Pamyatnykh (1999).
We consider various masses and chemical composition (X, Z). Moreover, two chemical mixtures were taken into account: the old one (GN93=Grevesse & Noels 1993) and the new one (A04=Asplund et al. 2004). We make accessible results obtained with the OPAL and OP opacity tables. For temperatures
log T ‹ 3.95 we use always the Aleksander & Ferguson (1994) opacities. The presented results were obtained for zero rotation velocity. In the near future we are going to extend the model grid in this parameter.
BIBLIOGRAFIA:
Asplund M., Grevesse N., Sauval A.J., 2004, ASP Conf. Ser, 336, 25
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
