El Eid M.F.; Meyer B.S.; The L.-S.
(Institute of Physics Publishing; CHICAGO1427 E 60TH ST, CHICAGO, IL 60637-2954 USA, 2004)
We present a detailed study of the evolution of massive stars of masses 15, 20, 25, and 30 M⊙ assuming solar-like initial chemical composition. The stellar sequences were evolved through the advanced burning phases up to ...