Zobrazeno 1 - 1
of 1
pro vyhledávání: '"Simon, Francesca E."'
Publikováno v:
Astrophys.J.562:521-527,2001
Stellar evolution models which include the effect of helium and heavy element diffusion have been calculated for initial iron abundances of [Fe/H] = -2.3, -2.1, -1.9 and -1.7. These models were calculated for a large variety of masses and three separ
Externí odkaz:
http://arxiv.org/abs/astro-ph/0108119
