Buch, Englisch, Band 179, 458 Seiten, HC runder Rücken kaschiert, Format (B × H): 160 mm x 241 mm, Gewicht: 1870 g
Buch, Englisch, Band 179, 458 Seiten, HC runder Rücken kaschiert, Format (B × H): 160 mm x 241 mm, Gewicht: 1870 g
Reihe: Astrophysics and Space Science Library
ISBN: 978-0-7923-1768-5
Verlag: Springer Netherlands
This book is divided into two parts. The first part deals with the general aspects of stellular structure and evolution including a chapter on numerical modelling. The second part deals with specific evolutionary aspects of single and binary stars with a variety of masses. The last chapter gives several models of stars with specific masses.
The book is intended as an introduction for students, as well as a reference for researchers.
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1: Introduction to the Stars.- 2: The Equations of Stellar Structure.- 3: The Equation of State.- 4: Nuclear Reation Rates.- 5: Nuclear Burning in Stellar Interiors.- 6: Astrophysical Opacities.- 7: Stellar Convection.- 8: Numerical Techniques.- 9: The Formation of Stars.- 10: Stellar Evolution during the Successive Nuclear Burning Phases.- 11: The Evolution of Low Mass Stars.- 12: The Evolution of Intermediate Stars (2.3 – 6 M).- 13: The Evolution of Massive Stars.- 14: Final Stages of Single Star Evolution.- 15: The Evolution of Binary Stars: General Considerations.- 16: The Evolution of Low and Intermediate Mass Binaries.- 17: The Evolution of Massive Close Binaries.- 18: Final Stages of Close Binary Evolution.- 19: Structure- and Evolutionary Models for Single and Binary Stars.- Annex: Polytropes.- A.1. Definition of polytropic relations.- A.2. The structure of polytropes.- A.3. The solution of the Lane-Emden equation.- A.4. Applications.- A. 5. Polytropic models.- A.6. The Chandrasekhar limiting mass.- References.- General References.- Literature per Chapter.