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Evolutionary processes in binary and multiple stars /

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 u...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor principal: Eggleton, P. P. (Peter P.), 1940-
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Cambridge, UK ; New York : Cambridge University Press, 2006.
Colección:Cambridge astrophysics series ; 40.
Temas:
Acceso en línea:Texto completo
Descripción
Sumario: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, first published in 2006, 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.
Descripción Física:1 online resource (viii, 322 pages) : illustrations
Bibliografía:Includes bibliographical references (pages 304-314) and indexes.
ISBN:9780511226298
0511226292
0511223080
9780511223082
9780511536205
0511536208
9786610550531
6610550530
1107166101
9781107166103
1280550538
9781280550539
0511225725
9780511225727
0511317832
9780511317835
0511225091
9780511225093