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Table of contents
1 Introduction
1.1 Historical review
1.2 Dust
2 Galaxies and dust
2.1 Galaxies
2.1.1 Introduction
2.1.2 Morphology
2.1.3 Kinematics
2.1.4 Stars
2.1.5 The interstellar medium
2.2 The Milky Way
2.2.1 The stellar component
2.2.2 The gaseous component
2.3 Dwarf galaxies
2.4 Dust
2.4.1 Effects on radiation
2.4.2 Composition
2.4.3 Box model
2.4.4 Production and destruction
2.4.5 Observations
3 Chemodynamical Code
3.1 Overview
3.1.1 Interaction of gas and stars
3.2 Dust Mass Evolution
3.2.1 The model
3.2.2 Production
3.2.3 Accretion
3.2.4 Destruction
4 First Result: The Milky Way
4.1 Simulation
4.2 Analysis
4.2.1 Radial distribution of dust
4.2.2 Vertical distribution of dust
4.2.3 Evolution of the dust-to-gas ratio
4.2.4 Evolution of the dust-to-oxygen ratio
4.2.5 Dust–metallicity diagram
4.2.6 Other diagrams
5 Second Result: The Dwarf Galaxies
5.1 Simulations
5.1.1 Dark matter
5.1.2 Stellar and gaseous components
5.1.3 Summary
5.2 Analysis
5.2.1 Evolution of the dust-to-oxygen ratio
5.2.2 Maps of the dust-to-oxygen ratio
5.2.3 Local correlation
5.2.4 Global correlation
6 Conclusion
A Improvement
B Parallelization
