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About Evolutionary Processes in Binary and Multiple Stars (Cambridge Astrophysics)
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.
Detailed Information
| Author: | Peter Eggleton |
|---|---|
| Publication Year: | 2006 |
| ISBN: | 9780511226298 |
| Pages: | 332 |
| Language: | English |
| File Size: | 8.819 |
| Format: | |
| Price: | FREE |
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