The s-process in AGB stars
About half of the solar abundances of elements heavier than iron are made by the slow neutron capture process (the s process) occurring in low and intermediate-mass asymptotic giant branch (AGB) stars. Elements are dredged from the core to the surface and
|Collections||ANU Research Publications|
|Source:||Proceedings of Science|
|01_Karakas_The_s-process_in_AGB_star_2010.pdf||113.74 kB||Adobe PDF||Request a copy|
Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.