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 |
|---|---|
| Date published: | 2010 |
| Type: | Conference paper |
| URI: | http://hdl.handle.net/1885/84037 |
| Source: | Proceedings of Science |
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| File | Description | Size | Format | Image |
|---|---|---|---|---|
| 01_Karakas_The_s-process_in_AGB_star_2010.pdf | 113.74 kB | Adobe PDF | Request a copy |
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