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Evolutionary Processes in Binary and Multiple Stars Hardback: 40 (Cambridge Astrophysics, Series Number 40) - Tapa dura
Sinopsis
This 2006 volume discusses the statistics of binary stars; the evolution of single stars; and interaction between multiple stars.
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Acerca del autor
Peter Eggleton is a physicist at the Lawrence Livermore National Laboratory in California.
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- EditorialCambridge University Press
- Año de publicación2006
- ISBN 10 0521855578
- ISBN 13 9780521855570
- EncuadernaciónTapa dura
- IdiomaInglés
- Número de páginas330
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Evolutionary Processes in Binary and Multiple Stars (Cambridge Astrophysics, Series Number 40)
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Cambridge University Press, 2006
ISBN 10: 0521855578
ISBN 13: 9780521855570
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Evolutionary Processes in Binary and Multiple Stars (Cambridge Astrophysics, Series Number 40)
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Cambridge University Press, 2006
ISBN 10: 0521855578
ISBN 13: 9780521855570
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Evolutionary Processes in Binary and Multiple Stars
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Hardcover. Condición: Brand New. 1st edition. 330 pages. 9.75x7.00x0.75 inches. In Stock. This item is printed on demand. Nº de ref. del artículo: __0521855578
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Evolutionary Processes in Binary and Multiple Stars
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Cambridge University Press, 2016
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ISBN 13: 9780521855570
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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. Nº de ref. del artículo: 446950734
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Evolutionary Processes in Binary and Multiple Stars (Hardcover)
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Cambridge University Press, Cambridge, 2006
ISBN 10: 0521855578
ISBN 13: 9780521855570
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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. 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. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability. Nº de ref. del artículo: 9780521855570
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Evolutionary Processes in Binary and Multiple Stars (Cambridge Astrophysics, Series Number 40)
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Evolutionary Processes in Binary and Multiple Stars
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Evolutionary Processes in Binary and Multiple Stars
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Evolutionary Processes in Binary and Multiple Stars (Hardcover)
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Cambridge University Press, Cambridge, 2006
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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. 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. Shipping may be from our Sydney, NSW warehouse or from our UK or US warehouse, depending on stock availability. Nº de ref. del artículo: 9780521855570
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Evolutionary Processes in Binary and Multiple Stars (Hardcover)
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Cambridge University Press, Cambridge, 2006
ISBN 10: 0521855578
ISBN 13: 9780521855570
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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. 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. Shipping may be from multiple locations in the US or from the UK, depending on stock availability. Nº de ref. del artículo: 9780521855570
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