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Synopsis
This self-contained astrophysics textbook for advanced undergraduates explores how stars form, what happens to them as they age, and what becomes of them when they die. Students can investigate the physical processes sustaining the energy output of stars during each stage of their evolution and which drive the progression from one stage to the next, and examine the relationship between different stages of stellar evolution and the production of the chemical elements. The textbook contains a wealth of worked examples and exercises with full solutions. Summaries, key facts and equations are clearly identified, and there are full colour illustrations throughout. Drawing on decades of experience in supported learning and independent study, this textbook is an ideal bridging text for astrophysics and physics majors looking to move on from the introductory texts. Accompanying resources to this textbook are available at: http://www.cambridge.org/features/astrophysics.
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Book Description
This self-contained astrophysics textbook for advanced undergraduates explores how stars form, what happens to them as they age, and what becomes of them when they die. It contains a wealth of worked examples, exercises with full solutions, full colour illustrations, and clearly identified summaries, key facts and equations.
About the Author
Sean Ryan is Professor of Astrophysics and Head of the School of Physics, Astronomy and Mathematics at the University of Hertfordshire. Prior to this he worked for the Open University, contributing to the development of courses in physics and astronomy.
Andrew Norton is Senior Lecturer in Physics and Astronomy in the Department of Physics and Astronomy, the Open University. He has authored teaching materials in physics and astronomy across the undergraduate curriculum, including twelve Open University study texts.
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- PublisherCambridge University Press
- Publication date2010
- ISBN 10 0521133203
- ISBN 13 9780521133203
- BindingPaperback
- LanguageEnglish
- Edition number1
- Number of pages236
- Rating
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Stellar Evolution and Nucleosynthesis
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