dc.contributor.author |
Mehio, Kawthar Rashid |
dc.date.accessioned |
2012-06-13T07:10:30Z |
dc.date.available |
2012-06-13T07:10:30Z |
dc.date.issued |
2007 |
dc.identifier.uri |
http://hdl.handle.net/10938/7392 |
dc.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 |
dc.description |
Bibliography : leaves 60-62. |
dc.description.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. |
dc.format.extent |
xi, 62 leaves : ill. (some col.) 30 cm. |
dc.language.iso |
eng |
dc.relation.ispartof |
Theses, Dissertations, and Projects |
dc.subject.classification |
T:004961 AUBNO |
dc.subject.lcsh |
Asymptotic giant branch stars |
dc.subject.lcsh |
Astrophysics |
dc.title |
Structure and evolution of asymptotic giant branch stars - by Kawthar Rashid Mehio |
dc.type |
Thesis |
dc.contributor.department |
American University of Beirut. Faculty of Arts and Sciences. Department of Physics |