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Evolutionary Processes in Binary and Multiple Stars

Evolutionary Processes in Binary and Multiple Stars

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"Evolutionary Processes in Binary and Multiple Stars" by Peter Eggleton is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

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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Best For: Students and researchers in astrophysics focusing on stellar evolution and binary star systems.
Focus: The evolutionary processes and interactions in binary and multiple star systems, including their stability and eventual instability.
Covers: Statistics of binary stars, nuclear reactions driving stellar evolution, and the impact of companions on stellar development.
Why It Matters: Understanding binary and multiple star evolution is crucial because these systems are common and their interactions significantly affect stellar life cycles and phenomena.

"Evolutionary Processes in Binary and Multiple Stars" by Peter Eggleton is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

Topic: Deep Sky & Solar System

Author: Peter Eggleton

Who this is for:

  • Astronomy students
  • Researchers and advanced hobbyists
  • Readers exploring space science topics

Why this book matters: It matters because it helps readers build a stronger understanding of astronomy concepts, observations, and scientific ideas related to space.

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.

AuthorPeter Eggleton
PublisherCambridge University Press
Published2006-07-20
ISBN-139780521855570
BindingHardcover
Pages330
LanguageEnglish
SubjectsScience
TopicDeep Sky & Solar System
SeriesCambridge Astrophysics

Format: Hardcover

Length: 330 pages

Language: English

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