Published by Cambridge University Press, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
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Published by Cambridge University Press, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
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Published by Cambridge University Press, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
Language: English
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Published by Cambridge University Press 2011-08-22, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
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Published by Cambridge University Press, Cambridge, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
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Paperback. Condition: new. Paperback. 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. Shipping may be from multiple locations in the US or from the UK, depending on stock availability.
Published by Cambridge University Press, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
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Published by Cambridge University Press, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
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Published by Cambridge University Press, Cambridge, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
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Add to basketPaperback. Condition: new. Paperback. 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. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability.
Published by Cambridge University Press, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
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Add to basketTaschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - This 2006 volume discusses the statistics of binary stars; the evolution of single stars; and interaction between multiple stars.
Published by Cambridge University Press, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Language: English
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Published by Cambridge University Press, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
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Published by Cambridge University Press, Cambridge, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
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Add to basketPaperback. Condition: new. Paperback. 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. Shipping may be from our Sydney, NSW warehouse or from our UK or US warehouse, depending on stock availability.
Published by Cambridge University Press, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
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Published by Cambridge University Press, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
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Published by Cambridge University Press, 2011
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Published by Cambridge University Press, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Language: English
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Published by Cambridge University Press, Cambridge, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Language: English
Seller: Grand Eagle Retail, Fairfield, OH, U.S.A.
Hardcover. Condition: 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.
Published by Cambridge University Press, Cambridge, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Language: English
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Add to basketHardcover. Condition: 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.
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Add to basketHardcover. Condition: Brand New. 1st edition. 330 pages. 9.75x7.00x0.75 inches. In Stock.
Published by Cambridge University Press, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Language: English
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Add to basketBuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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.
Published by Cambridge University Press, Cambridge, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Language: English
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Add to basketHardcover. Condition: 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.
Published by Cambridge University Press, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
Language: English
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Add to basketPaperback. Condition: Brand New. 330 pages. 9.61x6.69x0.75 inches. In Stock. This item is printed on demand.
Published by Cambridge University Press, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
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Add to basketPaperback / softback. Condition: New. This item is printed on demand. New copy - Usually dispatched within 5-9 working days 560.
Published by Cambridge University Press, 2011
ISBN 10: 1107403421 ISBN 13: 9781107403420
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Add to basketCondition: 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.
Published by Cambridge University Press, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Language: English
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Add to basketHardcover. Condition: Brand New. 1st edition. 330 pages. 9.75x7.00x0.75 inches. In Stock. This item is printed on demand.
Published by Cambridge University Press, 2016
ISBN 10: 0521855578 ISBN 13: 9780521855570
Language: English
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Add to basketGebunden. Condition: 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.