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Article Contents
- ABSTRACT
- 1.INTRODUCTION
- 2.DETAILED STAR FORMATION HISTORIES
- 2.1.Techniques: Synthetic CMD
analysis
- 2.1.1.An Example:
- 2.1.2.Testing the
Reliability:
- 2.2.Observations: Dwarf Galaxies in
the Local Group
- 2.2.1.Early-type Dwarf
Galaxies:
- 2.2.2.Late-type Dwarf
Galaxies:
- 2.2.3Ultra-faint dwarf
galaxies
- 2.2.4.The Small Magellanic
Cloud:
- 2.3.Beyond the Local Group
- 3.STELLAR KINEMATICS AND
METALLICITIES
- 3.1.Early-Type Dwarfs
- 3.1.1.Galactic dSphs:
- 3.1.2.More Distant dSphs:
- 3.1.3.Dwarf galaxies around M
31
- 3.2.Late-Type Dwarfs
- 3.3.Ultra-Faint Dwarfs
4.DETAILED ABUNDANCES OF RESOLVED
STARS
4.1.Dwarf Spheroidal Galaxies
4.1.1.alpha elements
4.1.2.Sodium and Nickel
4.1.3.Neutron-capture
elements
4.2.Ultra-Faint dwarf galaxies
4.3.Dwarf irregulars
5.CHEMICAL EVOLUTION MODELS
5.1.Explaining Low Metallicity
5.2.Galactic Winds
5.3.Modelling Individual systems
5.3.1.Standard Models
5.3.2.Chemo-dynamical models
5.3.3.Model predictions and
observed abundances
6.CONCLUDING REMARKS
REFERENCES