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
s processing in post-AGB and CH stars at low metallicity
โ Scribed by M. Busso; R. Gallino; C. Travaglio; M. Lugaro
- Publisher
- Elsevier Science
- Year
- 2001
- Tongue
- English
- Weight
- 148 KB
- Volume
- 688
- Category
- Article
- ISSN
- 0375-9474
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