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An Introduction to the Theory of Stellar Structure and Evolution
About this book
Using fundamental physics, the theory of stellar structure and evolution can predict how stars are born, how their complex internal structure changes, what nuclear fuel they burn, and their ultimate fate. This textbook is a stimulating introduction for undergraduates in astronomy, physics and applied mathematics, taking a course on the physics of stars. It uniquely emphasises the basic physical principles governing stellar structure and evolution. This second edition contains two new chapters on mass loss from stars and interacting binary stars, and new exercises. Clear and methodical, it explains the processes in simple terms, while maintaining mathematical rigour. Starting from general principles, this textbook leads students step-by-step to a global, comprehensive understanding of the subject. Fifty exercises and full solutions allow students to test their understanding. No prior knowledge of astronomy is required, and only a basic background in physics and mathematics is necessary.
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Information
Table of contents
- Cover
- Half Title
- Title Page
- Copyright
- Dedication
- Contents
- Preface to the second edition
- Preface to the first edition
- 1 Observational background and basic assumptions
- 2 The equations of stellar evolution
- 3 Elementary physics of gas and radiation in stellar interiors
- 4 Nuclear processes that take place in stars
- 5 Equilibrium stellar configurations β simple models
- 6 The stability of stars
- 7 The evolution of stars β a schematic picture
- 8 Mass loss from stars
- 9 The evolution of stars β a detailed picture
- 10 Exotic stars: supernovae, pulsars and black holes
- 11 Interacting binary stars
- 12 The stellar life cycle
- Appendix A β The equation of radiative transfer
- Appendix B β The equation of state for degenerate electrons
- Appendix C β Solutions to all the exercises
- Appendix D β Physical and astronomical constants and conversion factors
- Bibliography
- Index