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| dc.contributor.author | Mahmoud, Ghina Fawzi |
| dc.date.accessioned | 2012-06-13T07:14:47Z |
| dc.date.available | 2012-06-13T07:14:47Z |
| dc.date.issued | 2009 |
| dc.identifier.uri | http://hdl.handle.net/10938/7959 |
| dc.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" |
| dc.description | Bibliography : leaves 85-88. |
| dc.description.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 |
| dc.format.extent | 88 leaves : ill. 30 cm. |
| dc.language.iso | eng |
| dc.relation.ispartof | Theses, Dissertations, and Projects |
| dc.subject.classification | T:005314 AUBNO |
| dc.subject.lcsh | Stars -- Evolution |
| dc.title | Production of 13C in asymptotic giant branch stars - by Ghina Fawzi Mahmoud |
| dc.type | Thesis |
| dc.contributor.department | American University of Beirut. Faculty of Arts and Sciences. Department of Physics |
