Publication

2006 - Cambridge University Press, New York (State)

Language

English

Word Count

80,500 words, Guess

Page Count

322 pages

Physical Format

EBook

Identifiers

  • ISBN-100511223080
  • ISBN-139780511223082
  • OverDrive0634DCBF-FB59-4EC4-81F4-52890D66B861
  • OCLC Control Number159957466
  • Better World Books9780511226298
and 3 more
  • Better World Books9780511223082
  • Better World Books9780511224423
  • Open LibraryOL24287100M

Classifications

  • LCCQB821.E34 2006

Description

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 stably 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. Some of the interactions discussed are Roche-lobe overflow, tidal friction, gravitational radiation, magnetic activity driven by rapid rotation, stellar winds, magnetic braking, and the influence of a distant third body on a close binary orbit. A series of mathematical appendices gives a concise but full account of the mathematics of these processes.

Subjects

Other Editions

  • Evolutionary Processes in Binary and Multiple StarsEBookCambridge University Press2006

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