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Intro; Supervisor's Foreword; Parts of this thesis have been published in the following journal articles:; Acknowledgements; Contents; 1 Introduction; 1.1 Astrophysical Sites of Elements; 1.1.1 Solar System Abundances; 1.1.2 Nucleosynthesis; 1.1.3 Astrophysical Sites of Heavy Elements; 1.2 The Local Group Galaxies; 1.2.1 The Observed Local Group Galaxies; 1.2.2 Chemical Abundances of Local Group Dwarf Galaxies; 1.3 Formation and Evolution of Galaxies; 1.3.1 Galaxy Formation; 1.3.2 Galactic Chemical Evolution; 1.4 This Book; References; 2 Methods for Simulations of Galaxy Formation

2.1 The N-body and Smoothed Particle Hydrodynamics Code, asura2.2 Feedback from Massive Stars; 2.2.1 Models of Core-Collapse Supernovae; 2.2.2 Models of Electron-Capture Supernovae; 2.2.3 Models of Neutron Star Mergers; 2.3 Feedback Models of Intermediate and Low Mass Stars; 2.4 Nucleosynthesis Yields of Supernovae; 2.5 Ejection of Metals; 2.6 Mixing of Metals; 2.6.1 Definition of Metallicity in Stars; 2.6.2 Metal Mixing Models for Gas Particles; 2.7 Summary; References; 3 Chemodynamical Evolution of Dwarf Galaxies; 3.1 Models of Dwarf Spheroidal Galaxies

6.3 Effects of the Metal Mixing on the Enrichment of r-Process Elements6.4 Efficiency of Metal Mixing; 6.5 Summary; References; 7 Enrichment of r-Process Elements in a Cosmological Context; 7.1 Enrichment of r-Process Elements and Galaxy Formation; 7.2 Cosmological Zoom-In Simulations; 7.3 Enrichment of r-Process Elements in Cosmological Simulations; 7.4 The Origin of r-Process Enhanced Stars; 7.5 Summary; References; 8 Conclusions and Future Prospects; 8.1 Conclusions; 8.2 Future Prospects; 8.2.1 Multi-messenger Astronomy; 8.2.2 Star-By-Star Simulations

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