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Revista mexicana de física
Print version ISSN 0035-001X
Rev. mex. fis. vol.52 suppl.1 México Jan. 2006
The 19F(α,p1γ)22Ne reaction and the abundance of fluorine in Asymptotic Giant Branch (AGB) stars.
C. Ugalde, A. Couture, J. Görres, E. Stech, and M. Wiescher
Department of Physics, University of Notre Dame, Notre Dame, IN 46556, USA
Recibido el 31 de enero de 2005
Aceptado el 3 de abril de 2005
Abstract
The 19F(α,p1γ) reaction was investigated in the energy range E α= 1.15 2.00 MeV. Eight resonances were found in the gamma excitation curve, five of which were not observed before. Energy and strength of the resonances were obtained and compared well to values available elsewhere (Kuperus, J., Physica 31, (1965) 1603).
Keywords: Asymptotic Giant Branch; Nuclear Astrphysics; Fluorine.
Resumen
La reacción 19F(α,p1γ) ha sido investigada en el intervalo de energía Eα= 1.15 2.00 MeV. Se observaron ocho resonancias en la función de excitación, de las que cinco eran desconocidas a la fecha. Las energías e intensidades de las resonancias fueron obtenidas y son comparables con otros valores medidos previamente (Kuperus, J., Physica 31, (1965) 1603).
Descriptores: Astrofísica nuclear, Fluor.
PACS: 26.50.+x; 27.20.+n
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