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19 April 2024 |
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Article overview
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Hydrogen burning of 17O in classical novae | A Chafa
; V Tatischeff
; P Aguer
; S Barhoumi
; A Coc
; F Garrido
; M Hernanz
; J José
; J Kiener
; A Lefebvre-Schuhl
; S Ouichaoui
; N de Séréville
; J-P Thibaud
; | Date: |
15 Jul 2005 | Journal: | Phys Rev Lett, 95 (3), 031101 | Abstract: | We report on the observation of a previously unknown resonance at E(lab)(R)=194.1+/-0.6 keV in the 17O(p,alpha)14N reaction, with a measured resonance strength omegagamma(palpha)=1.6 +/- 0.2 meV. We studied in the same experiment the 17O(p,gamma)18F reaction by an activation method and the resonance-strength ratio was found to be omegagamma(palpha)/omegagamma(pgamma) = 470 +/- 50. The corresponding excitation energy in the 18F compound nucleus was determined to be 5789.8 +/- 0.3 keV by gamma-ray measurements using the 14N(alpha, gamma)18F reaction. These new resonance properties have important consequences for 17O nucleosynthesis and gamma-ray astronomy of classical novae. | Source: | PubMed, pmid16090732 | Services: | Forum | Review | Favorites |
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