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,
The G-dwarf problem in the Galaxy
โ Scribed by R. Caimmi
- Publisher
- Elsevier Science
- Year
- 2008
- Tongue
- English
- Weight
- 757 KB
- Volume
- 13
- Category
- Article
- ISSN
- 1384-1076
No coin nor oath required. For personal study only.
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 three different samples involving (i) local thick disk stars derived from Gliese and scaled in situ samples within the range,
๐ SIMILAR VOLUMES
## Abstract We study the properties of the dwarf galaxy population in the nearby interacting M81 group of galaxies. In particular, we are deriving the metallicity distribution functions, the ages and the star formation histories of these dwarf galaxies based on data from the Hubble Space Telescope'