Evolutionary processes binary stars (70 Ergebnisse)

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PF. Zustand: New.

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Zustand: New. This 2006 volume discusses the statistics of binary stars; the evolution of single stars; and interaction between multiple stars. Series: Cambridge Astrophysics. Num Pages: 332 pages, Illustrations. BIC Classification: PGM; PHVB. Category: (P) Professional & Vocational. Dimension: 246 x 170 x 18. Weight in Grams: 548. . 2011. Paperback. . . . .…

Zustand: New. pp. 332.

Zustand: New. This 2006 volume discusses the statistics of binary stars; the evolution of single stars; and interaction between multiple stars. Series: Cambridge Astrophysics. Num Pages: 332 pages, Illustrations. BIC Classification: PGM; PHVB. Category: (P) Professional & Vocational. Dimension: 246 x 170 x 18. Weight in Grams: 548. . 2011. Paperback. . . . . Books ship from the US and Ireland.…

Couverture souple. Zustand: bon. R260269808: 1992. In-8. Broché. Très bon état, Couv. convenable, Dos satisfaisant, Intérieur frais. 530 pages augmentées de quelques figures en noir et blanc dans texte. . . . Classification Dewey : 420-Langue anglaise. Anglo-saxon.

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Zustand: New.

Zustand: New. In English.

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Zustand: New.

Zustand: New. This 2006 volume discusses the statistics of binary stars; the evolution of single stars; and interaction between multiple stars. Series: Cambridge Astrophysics. Num Pages: 332 pages, 52 b/w illus. 28 tables. BIC Classification: PGM. Category: (P) Professional & Vocational. Dimension: 247 x 174 x 19. Weight in Grams: 828. . 2006. Illustrated. hardcover. . . . . …

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Zustand: New.

Zustand: New. In English.

Zustand: New. In English.

Zustand: New.

Hardback. Zustand: New. 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.…

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Zustand: New. This 2006 volume discusses the statistics of binary stars; the evolution of single stars; and interaction between multiple stars. Series: Cambridge Astrophysics. Num Pages: 332 pages, 52 b/w illus. 28 tables. BIC Classification: PGM. Category: (P) Professional & Vocational. Dimension: 247 x 174 x 19. Weight in Grams: 828. . 2006. Illustrated. hardcover. . . . . Books ship from the US and Ireland. …

Hardcover. Zustand: Brand New. 1st edition. 330 pages. 9.75x7.00x0.75 inches. In Stock.

Zustand: New. Proceedings of the NATO Advanced Study Institute, Cambridge, United Kingdom, July 10-21, 1995 Editor(s): Wijers, Ralph A. M. J.; Davies, Melvyn B. (Institute of Astronomy, University of Cambridge, UK); Tout, Christopher A. (Institute of Astronomy, University of Cambridge, UK). Series: NATO Science Series C. Num Pages: 412 pages, biography. BIC Classification: PGM; PHVB. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 234 x 156 x 25. Weight in Grams: 796. . 1996. Hardback. . . . . …

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Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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.…

Hardback. Zustand: New. 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.…

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Paperback. Zustand: Brand New. 412 pages. 9.44x6.31x1.00 inches. In Stock.

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