The s-process in AGB stars
Karakas, Amanda; Lugaro, Maria
Description
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 |
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Date published: | 2010 |
Type: | Conference paper |
URI: | http://hdl.handle.net/1885/84037 |
Source: | Proceedings of Science |
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01_Karakas_The_s-process_in_AGB_star_2010.pdf | 113.74 kB | Adobe PDF | Request a copy |
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