The Impact of the18F(α,p)21Ne Reaction on Asymptotic Giant Branch Nucleosynthesis

2007/12/18 by Amanda Karakas, Amanda I. Karakas, Hye Young Lee +5 · 1 citation
Environmental Science · Physics and Astronomy · #Nuclear Physics and Applications #Nuclear physics research studies #Radioactive contamination and transfer #astro-ph

paper · pdf · doi:10.1086/528840

9 pages, accepted for publication in ApJ

arxiv created 2007/12/18 · openalex publication_date 2008/04/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

We present detailed models of low- and intermediate-mass asymptotic giant branch (AGB) stars with and without the 18F(α, p) 21Ne reaction included in the nuclear network, where the rate for this reaction has been recently experimentally evaluated for the

Citations

• Fluorine Abundances in the Large Magellanic Cloud and Centauri: Evidence for Neutrino Nucleosynthesis?
• The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis
• Evolution of Asymptotic Giant Branch Stars
• Nucleosynthesis in Asymptotic Giant Branch Stars: Relevance for Galactic Enrichment and Solar System Formation
• The Discovery of Fluorine in Cool Extreme Helium Stars
• CARBON STARS

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