The uncertainties in the22Ne+α-capture reaction rates and the production of the heavy magnesium isotopes in asymptotic giant branch stars of intermediate mass

Astrophysical Journal

Volumn 643, Issue 1 I, 2006, Pages 471-483

  Karakas, A I ^a,d,e,f   Lugaro, M A ^b,g   Wiescher, M ^c   Gorres J ^c   Ugalde, C ^c,h,i  

^a SAINT MARY S UNIVERSITY   (Canada)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c UNIVERSITY OF NOTRE DAME   (United States)

^d SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

^e MONASH UNIVERSITY   (Australia)

^f MCMASTER UNIVERSITY   (Canada)

^g UTRECHT UNIVERSITY   (Netherlands)

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

ⁱ TRIANGLE UNIVERSITIES NUCLEAR LABORATORY   (United States)

Author keywords

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

Indexed keywords

EID: 33745824585     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/502793     Document Type: Article

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