Production of 13C in asymptotic giant branch stars - by Ghina Fawzi Mahmoud
| dc.contributor.author | Mahmoud, Ghina Fawzi | |
| dc.contributor.department | American University of Beirut. Faculty of Arts and Sciences. Department of Physics | |
| dc.date | 2009 | |
| dc.date.accessioned | 2012-06-13T07:14:47Z | |
| dc.date.available | 2012-06-13T07:14:47Z | |
| dc.date.issued | 2009 | |
| 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.identifier.uri | http://hdl.handle.net/10938/7959 | |
| dc.language.iso | en | |
| 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 |