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THE FLUORINE DESTRUCTION IN STARS: FIRST EXPERIMENTAL STUDY OF THE (19)F(p, alpha(0))(16)O REACTION AT ASTROPHYSICAL ENERGIES

  1. 1.
    SYSNO ASEP0364991
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleTHE FLUORINE DESTRUCTION IN STARS: FIRST EXPERIMENTAL STUDY OF THE (19)F(p, alpha(0))(16)O REACTION AT ASTROPHYSICAL ENERGIES
    Author(s) La Cognata, M. (IT)
    Mukhamedzhanov, A. M. (US)
    Spitaleri, C. (IT)
    Indelicato, I. (IT)
    Aliotta, M. (IT)
    Burjan, Václav (UJF-V) RID, ORCID, SAI
    Cherubini, S. (IT)
    Coc, A. (FR)
    Gulino, M. (IT)
    Hons, Zdeněk (UJF-V) RID, ORCID
    Kiss, G.G. (IT)
    Kroha, Václav (UJF-V) RID
    Lamia, L. (IT)
    Mrázek, Jaromír (UJF-V) RID, ORCID, SAI
    Palmerini, S. (IT)
    Piskoř, Štěpán (UJF-V) RID
    Pizzone, R. G. (IT)
    Puglia, S. M. R. (IT)
    Rapisarda, G. G. (IT)
    Romano, S. (IT)
    Sergi, M. L. (IT)
    Tumino, A. (IT)
    Number of authors22
    Source TitleAstrophysical Journal Letters. - : Institute of Physics Publishing - ISSN 2041-8205
    Roč. 739, č. 2 (2011), L54
    Number of pages1 s.
    Languageeng - English
    CountryUS - United States
    KeywordsASYMPTOTIC GIANT BRANCH ; CORONAE-BOREALIS STARS ; NUCLEAR ASTROPHYSICS ; COULOMB BARRIER ; CROSS-SECTION ; LOW-MASS ; NUCLEOSYNTHESIS ; CARBON
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    R&D ProjectsLC07050 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    GAP203/10/0310 GA ČR - Czech Science Foundation (CSF)
    CEZAV0Z10480505 - UJF-V (2005-2011)
    UT WOS000294997600020
    DOI10.1088/2041-8205/739/2/L54
    AnnotationThe (19)F(p, alpha)(16)O reaction is an important fluorine destruction channel in the proton-rich outer layers of asymptotic giant branch (AGB) stars and it might also play a role in hydrogen-deficient post-AGB star nucleosynthesis. So far, available direct measurements do not reach the energy region of astrophysical interest (E(cm) less than or similar to 300 keV), because of the hindrance effect of the Coulomb barrier.
    WorkplaceNuclear Physics Institute
    ContactMarkéta Sommerová, sommerova@ujf.cas.cz, Tel.: 266 173 228
    Year of Publishing2012
Number of the records: 1  

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