Evolutionary Processes in Binary and Multiple Stars
Part of Cambridge Astrophysics
- Author: Peter Eggleton, Lawrence Livermore National Laboratory, California
- Date Published: July 2006
- availability: Available
- format: Hardback
- isbn: 9780521855570
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Binary systems of stars are as common as single stars. Stars evolve primarily by nuclear reactions in their interiors, but a star with a binary companion can also have its evolution influenced by the companion. Multiple star systems can exist in a stable state for millions of years, but can ultimately become unstable as one star grows in radius until it engulfs another. This volume discusses the statistics of binary stars; the evolution of single stars; and several of the most important kinds of interaction between two (and even three or more) stars. A series of mathematical appendices provides a concise but complete account of the mathematics of these processes.
Read more- Peter Eggleton is one of the most knowledgeable experts in binary star evolution
- The only comprehensive reference work on binary star evolution, this book takes the reader right up to the frontiers of research
- Includes several mathematical appendices summarizing the necessary methods from the literature as a unified whole, using a consistent notation
Reviews & endorsements
Review of the hardback: '… I know of no book quite like Peter Eggleton's monograph, which describes in great detail stellar evolution in the context of binary and to some extent multiple stars, but also gives a masterly and comprehensive one-chapter summary of single-star evolution, in a very concise style. Anyone who masters the contents will have a deep understanding of the processes involved and of the approximations that are necessary to make progress. … the writing is clear and readable … the text is full of nice phrases that are accessible to everyone … A nice feature of the book, that will make it more accessible to non-experts, is that the detailed mathematical justifications have mostly been placed in the appendices that take up the last 50 pages of the book … a remarkable book … it is authoritative and comprehensive and will be a fruitful source of ideas for those working in the field. It should also persuade our extragalactic colleagues that stellar evolution is still a topic with lots of interesting unsolved problems.' The Observatory
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17th Oct 2024 by UName-818593
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×Product details
- Date Published: July 2006
- format: Hardback
- isbn: 9780521855570
- length: 332 pages
- dimensions: 244 x 170 x 19 mm
- weight: 0.83kg
- availability: Available
Table of Contents
1. Introduction
2. Evolution of single stars
3. Binary interaction: conservative processes
4. Slow non-conservative processes
5. Rapid non-conservative processes
6. Accretion by the companion
Appendices.
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