Evolutionary Processes in Binary and Multiple Stars
Peter P. Eggleton - Evolutionary Processes in Binary and Multiple Stars
Publisher: Cаmbridge Univеrsity Prеss | 2006-07-24 | ISBN: 0521855578 | PDF | 330 pages | 9.25 MB
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.
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Multiple Star Systems Binary Companion Mbridge Multiple Stars Binary Stars Rsity Binary Systems Adobe Reader Evolutionary Processes Stable State Downloaded File Nuclear Reactions Appendices Radius Interaction Mathematics Evolution Ss Statistics Publisher
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