The astrophysically important 3+ state in 18Ne and the 17F(p, γ)18Ne stellar rate

Physical Review C - Nuclear Physics

Volumn 62, Issue 5, 2000, Pages 558041-5580414

  Bardayan, D W ^a,b,c   Blackmon, J C ^a   Brune, C R ^c   Champagne, A E ^c   Chen, A A ^b   Cox, J M ^d   Davinson, T ^e   Hansper, V Y ^a,c,i   Hofstee, M A ^f   Johnson, B A ^d   Kozub, R L ^d   Ma, Z ^a,g,h   Parker, P D ^b   Pierce, D E ^a   Rabban, M T ^a   Shotter, A C ^e   Smith, M S ^a   Swartz, K B ^b   Visser, D W ^b   Woods, P J ^e  

^a OAK RIDGE NATIONAL LABORATORY   (United States)

^b YALE UNIVERSITY   (United States)

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

^d TENNESSEE TECHNOLOGICAL UNIVERSITY   (United States)

^e UNIVERSITY OF EDINBURGH   (United Kingdom)

^f Department of Geology and Geological Engineering   (United States)

^g CHINA INSTITUTE OF ATOMIC ENERGY   (China)

^h JOINT INSTITUTE FOR HEAVY ION RESEARCH   (United States)

ⁱ AARHUS UNIVERSITY   (Denmark)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 12944265466     PISSN: 05562813     EISSN: 1089490X     Source Type: Journal    
DOI: 10.1103/PhysRevC.62.055804     Document Type: Article

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