Hot Bottom Burning in Asymptotic Giant Branch Stars
this paper, we want to discuss only the situation with Al. This is found in many grains, such as SiC (believed to form in the carbon-rich atmospheres of Carbon stars), graphite (a very complex and heterogeneous sample of grains) and corundum (Al 2 O 3 ...
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History of individual presolar SiC grains revealed by stellar winds. [PDF]
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Structure and evolution of asymptotic giant branch stars - by Kawthar Rashid Mehio
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.
Mehio, Kawthar Rashid
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