Structure and evolution of asymptotic giant branch stars - by Kawthar Rashid Mehio
Abstract
In this thesis, we focus on the study of structure and evolution of low mass sta rs of masses 2M (solar) and 3M (solar) and initial solar-like composition. The m ost interesting evolutionary phase of such stars is the Asymptotic Giant Branch (AGB) stage.
Description
Thesis (M.S.)--American University of Beirut, Dept.of Physics, 2007.;"Advisor: Dr. Mounib El Eid, Professor, Department of Physics--Member of Committee: Dr. Leonid Klushin, Professor, Department of Physics--Member of Committee: Dr. Jihad Touma, Associate
Bibliography : leaves 60-62.
Bibliography : leaves 60-62.