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 emphasizes 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 rigor. 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.

Reviews & endorsements

“The unique feature of this book is the emphasis it places, throughout, on the basic physical principles governing stellar evolution. The processes are always explained in the simplest terms, while maintaining full mathematical rigour … This textbook provides a stimulating introduction for undergraduates in astronomy, physics, planetary science, and applied mathematics who are taking a course on the physics of stars. Because this book requires only basic undergraduate physics and mathematics and no prior knowledge of astronomy it may be read by advanced amateurs as well.” – Orion

Author

Dina Prialnik, Tel-Aviv University
Dina Prialnik is a Professor of Planetary Physics at Tel Aviv University. Her research interests lie in stellar evolution; the structure and evolution of cataclysmic variables, comet nuclei and other small Solar System bodies; and the evolution of planets.

Table of Contents

1. Observations and assumptions
2. Equations of stellar evolution
3. Physics of gas and radiation
4. Nuclear processes
5. Equilibrium – simple models
6. Stability of stars
7. Evolution of stars – schematic picture
8. Mass loss from stars
9. The evolution of stars – a detailed picture
10. Exotic stars: supernovae, pulsars, black holes
11. Interacting binary stars
12. The stellar life cycle
Appendixes
References
Index.