Reaction rate uncertainties and 26Al in AGB silicon carbide stardust

Astronomy and Astrophysics

Volumn 478, Issue 2, 2008, Pages 521-526

  Van Raai, M A ^a   Lugaro, M ^a,b   Karakas, A I ^c   Iliadis, C ^d,e  

^a UTRECHT UNIVERSITY   (Netherlands)

^b MONASH UNIVERSITY   (Australia)

^c AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^d University of North Carolina at Chapel Hill   (United States)

^e Triangle Universities   (United States)

Author keywords

Nuclear reactions, nucleosynthesis, abundances; Stars: AGB and post AGB

Indexed keywords

AGB STARS; AL COMPOSITION; ASYMPTOTIC GIANT BRANCH STARS; CARBON RICH; DIFFERENT MASS; FOUR-ORDER; LABORATORY ANALYSIS; LOWER LIMITS; METALLICITIES; MODEL PREDICTION; NUCLEAR EXPERIMENTS; NUCLEAR REACTIONS , NUCLEOSYNTHESIS , ABUNDANCES; PRESOLAR GRAIN; RADIOACTIVE NUCLEI; RECOMMENDED VALUES; SIC GRAINS; STARS:AGB AND POST AGB; UPPER LIMITS;

REACTION RATES; SILICON; SILICON CARBIDE; STARS; TRACE ELEMENTS; UNCERTAINTY ANALYSIS;

ALUMINUM;

EID: 51649096771     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078307     Document Type: Article

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