Results from existing models of s-processing in red giants are compared with key observed abundances in population I and II AGB stars. Population I giants are particularly important for getting constraints on the neutron density (from Rb/Sr ratios), while population II AGB's provide clues to underst
✦ LIBER ✦
s‐Process Nucleosynthesis in Low‐Mass AGB Stars at Different Metallicities
✍ Scribed by Cristallo, S.
- Book ID
- 123914587
- Publisher
- University of Chicago Press
- Year
- 2006
- Tongue
- English
- Weight
- 84 KB
- Volume
- 118
- Category
- Article
- ISSN
- 0004-6280
- DOI
- 10.1086/507774
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