The Impact of the 18F(α,p)21Ne Reaction on Asymptotic Giant Branch Nucleosynthesi
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
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Karakas_The_Impact_of_the_18F(α,p)21Ne_2008.pdf||1.13 MB||Adobe PDF||Request a copy|
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