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Physical Processes and Numerical Methods Common to Structure Formations in Astrophysics: | |
The physics of turbulence | |
The numerical simulation of turbulence | |
Numerical methods for radiation magnetohydrodynamics in astrophysics | |
The role of jets in the formation of planets, stars, and galaxies | |
Advanced numerical methods in astrophysical fluid dynamics | |
Structure and Star Formation in the Primordial Universe: | |
New frontiers in cosmology and galaxy formation challenges for the future | |
Galaxy formation physics | |
First stars formation, evolution, feedback effects | |
Contemporary Star and Brown Dwarf Formation: a) Cloud Formation and Fragmentation: | |
Diffuse interstellar medium and the formation of molecular clouds | |
The formation of distributed and clustered stars in molecular clouds | |
b) Core Fragmentation and Star Formation: | |
The formation and evolution of prestellar cores | |
Models for the formation of massive stars | |
Protoplanetary Disks and Planet Formation | |
Observational properties of disks and young stellar objects | |
Structure and dynamics of protoplanetary disks | |
Planet formation and evolution theory and observation | |
Planet formation assembling the puzzle | |
Summary: | |
Open issues in small- and large-scale structure formation | |
Final word | |
Table of Contents provided by Publisher. All Rights Reserved. |
The New copy of this book will include any supplemental materials advertised. Please check the title of the book to determine if it should include any access cards, study guides, lab manuals, CDs, etc.
The Used, Rental and eBook copies of this book are not guaranteed to include any supplemental materials. Typically, only the book itself is included. This is true even if the title states it includes any access cards, study guides, lab manuals, CDs, etc.