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Structure and evolution of asymptotic giant branch stars - by Kawthar Rashid Mehio

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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


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