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| dc.contributor.author | Shaya, Wissam Shafic |
| dc.date.accessioned | 2012-06-13T06:45:50Z |
| dc.date.available | 2012-06-13T06:45:50Z |
| dc.date.issued | 1999 |
| dc.identifier.uri | http://hdl.handle.net/10938/5686 |
| dc.description | Thesis (M.S.)--American University of Beirut. Department of Physics, 1999;"Advisor: Dr. Mounib El Eid, Professor, Physics--Member of Committee: Dr. Leonid Klushin, Professor,Physics--Member of Committee: Dr. Michel Abou Ghantous, Professor, Physics" |
| dc.description | Bibliography : leaves 111-113 |
| dc.description.abstract | Element formation in stars (the so-called nucleosynthesis) due to thermonuclear reactions is a powerful diagnostic of the physical processes occurring in their deep interiors. An important physical process in stars is the convective mixing which can expos |
| dc.format.extent | xii, 113 leaves : ill., tables |
| dc.language.iso | eng |
| dc.relation.ispartof | Theses, Dissertations, and Projects |
| dc.subject.classification | T:003974 AUBNO |
| dc.subject.lcsh | Stars -- Formation |
| dc.title | Element formation in giant and supergiant stars - by Wissam Shafic Shaya |
| dc.type | Thesis |
| dc.contributor.department | American University of Beirut. Faculty of Arts and Sciences. Department of Physics |
