Production of 13C in asymptotic giant branch stars - by Ghina Fawzi Mahmoud
Abstract
We present stellar model calculations for 3 and 3.5 solar mass stars with solar -like composition. These stars were evolved from the main sequence up to the evo lutionary phase known as Asymptotic Giant Branch (AGB). This mass range is impor tant because
Description
Thesis (M.S.)--American University of Beirut, Dept. of Physics, 2009.;"Advisor : Dr. Mounib El Eid, Professor , Physics--Member of Committee : Dr. Malek Tabbal, Professor , Physics--Member of Committee : Dr. Ghassan Antar, Assistant Professor ,Physics"
Bibliography : leaves 85-88.
Bibliography : leaves 85-88.