This paper has two parts: one about observational constraints, and the other about chemical evolution models. In the first part, the empirical differential metallicity distribution (EDMD) is deduced from three different samples involving (i) local thick disk stars derived from Gliese and scaled in s
โฆ LIBER โฆ
The G-dwarf problem in the Galactic spheroid
โ Scribed by R. Caimmi
- Publisher
- Elsevier Science
- Year
- 2007
- Tongue
- English
- Weight
- 897 KB
- Volume
- 12
- Category
- Article
- ISSN
- 1384-1076
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โฆ Synopsis
This paper has two parts: one about observational constraints, and the other about chemical evolution models. In the first part, the empirical differential metallicity distribution (EDMD) is deduced from two different samples involving (i) 268 K-giant bulge stars [Sadler,
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