Isbn: 9780521855570 - evolutionary processes in binary and multiple stars hardback: 40 (cambridge astrophysics, series number 40) (17 resultados)

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Condición: 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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Hardback. Condición: 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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Condición: 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. …

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Buch. Condición: 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. Condición: 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. …

Gebunden. Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. This 2006 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 gives a concise but full account.…

Hardcover. Condición: new. Hardcover. 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. This 2006 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 gives a concise but full account of the mathematics of these processes. This item is printed on demand. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability.…

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Buch. Condición: Neu. Evolutionary Processes in Binary and Multiple Stars | Peter Eggleton | Buch | Gebunden | Englisch | 2016 | Cambridge University Press | EAN 9780521855570 | Verantwortliche Person für die EU: Libri GmbH, Europaallee 1, 36244 Bad Hersfeld, gpsr[at]libri[dot]de | Anbieter: preigu Print on Demand.…