The inelastic component of the key astrophysical resonance (1 -, E x =6.15 MeV) in the 14 O(α,p) 17 F reaction has been studied by using the resonant scattering of 17 F+p. The experiment was done at REX-ISOLDE CERN with the Miniball setup. The thick target method in inverse kinematics was utilized i
Study of Stellar Reactions in Explosive Hydrogen Burning with CRIB
✍ Scribed by S. Kubono; T. Teranishi; M. Notani; H. Yamaguchi; A. Saito; J.J. He; M. Wakabayashi; H. Fujikawa; G. Amadio; H. Baba; T. Fukuchi; S. Shimoura; S. Michimasa; S. Nishimura; M. Nishimura; Y. Gono; A. Odahara; S. Kato; J.Y. Moon; J.H. Lee; C.S. Lee; J.C. Kim; K.I. Hahn; T. Ishikawa; T. Hashimoto; H. Ishiyama; Y.X. Watanabe; M.H. Tanaka; H. Miyatake; Zs. Fülöp; V. Guimarães; R. Lichtenthaler
- Publisher
- Elsevier Science
- Year
- 2005
- Tongue
- English
- Weight
- 177 KB
- Volume
- 758
- Category
- Article
- ISSN
- 0375-9474
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