A. Tattersall

Stardust grains that originated in ancient stars and supernovae are recovered from meteorites and carry the detailed composition of their astronomical sites of origin. We present e…

nucl-ex2020★ 58 cited

Re-evaluation of the $^{22}$ Ne( $α, γ$ ) $^{26}$ Mg and $^{22}$ Ne( $α, n$ ) $^{25}$ Mg reaction rates

Philip Adsley, Umberto Battino, Andreas Best +11

The competing $^{22}$ Ne( $α, γ$ ) $^{26}$ Mg and $^{22}$ Ne( $α, n$ ) $^{25}$ Mg reactions control the production of neutrons for the weak $s$ -process in massive and AGB stars. In both system…

Origin of large meteoritic SiC stardust grains in metal-rich AGB stars

Re-evaluation of the 22Ne(α,γ)26Mg and 22Ne(α,n)25Mg reaction rates

Re-evaluation of the $^{22}$ Ne( $α, γ$ ) $^{26}$ Mg and $^{22}$ Ne( $α, n$ ) $^{25}$ Mg reaction rates