26gAl(p,γ)27Si at Stellar Temperatures

Published: May 2015 Bardayan

Lead Author(s): S.D. Pain

The rate of the 26gAl(p,γ)27Si reaction at stellar temperatures determines, in part, the contributions that various stellar events make to the observed 26gAl g-ray flux from the Galactic center.  The rate has been constrained via an 26gAl(d,p)27Al study at the ORNL Holifield Radioactive Ion Beam Facility. Learn more

Publication: Constraint of the Astrophysical 26gAl(p,γ)27Si Destruction Rate at Stellar Temperatures