Librería: AwesomeBooks, Wallingford, Reino Unido
EUR 42,05
Cantidad disponible: 2 disponibles
Añadir al carritoHardcover. Condición: Very Good. Evolutionary Processes in Binary and Multiple Stars: 40 (Cambridge Astrophysics, Series Number 40) This book is in very good condition and will be shipped within 24 hours of ordering. The cover may have some limited signs of wear but the pages are clean, intact and the spine remains undamaged. This book has clearly been well maintained and looked after thus far. Money back guarantee if you are not satisfied. See all our books here, order more than 1 book and get discounted shipping.
Librería: Bahamut Media, Reading, Reino Unido
EUR 42,05
Cantidad disponible: 2 disponibles
Añadir al carritoHardcover. Condición: Very Good. This book is in very good condition and will be shipped within 24 hours of ordering. The cover may have some limited signs of wear but the pages are clean, intact and the spine remains undamaged. This book has clearly been well maintained and looked after thus far. Money back guarantee if you are not satisfied. See all our books here, order more than 1 book and get discounted shipping.
Idioma: Inglés
Publicado por Cambridge University Press, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Librería: GreatBookPrices, Columbia, MD, Estados Unidos de America
EUR 185,24
Cantidad disponible: Más de 20 disponibles
Añadir al carritoCondición: New.
Idioma: Inglés
Publicado por Cambridge University Press, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Librería: Ria Christie Collections, Uxbridge, Reino Unido
EUR 178,78
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Añadir al carritoCondición: New. In.
Idioma: Inglés
Publicado por Cambridge University Press, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Librería: GreatBookPricesUK, Woodford Green, Reino Unido
EUR 178,77
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Añadir al carritoCondición: New.
Idioma: Inglés
Publicado por Cambridge University Press, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Librería: GreatBookPrices, Columbia, MD, Estados Unidos de America
EUR 200,79
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Añadir al carritoCondición: As New. Unread book in perfect condition.
Idioma: Inglés
Publicado por Cambridge University Press, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Librería: GreatBookPricesUK, Woodford Green, Reino Unido
EUR 204,74
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Añadir al carritoCondición: As New. Unread book in perfect condition.
Idioma: Inglés
Publicado por CAMBRIDGE UNIVERSITY PRESS, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Librería: UK BOOKS STORE, London, LONDO, Reino Unido
EUR 248,70
Cantidad disponible: 1 disponibles
Añadir al carritoCondición: New. Brand New! Fast Delivery This is an International Edition and ship within 24-48 hours. Deliver by FedEx and Dhl, & Aramex, UPS, & USPS and we do accept APO and PO BOX Addresses. Order can be delivered worldwide within 7-12 days and we do have flat rate for up to 2LB. Extra shipping charges will be requested if the Book weight is more than 5 LB. This Item May be shipped from India, United states & United Kingdom. Depending on your location and availability.
Librería: Revaluation Books, Exeter, Reino Unido
EUR 247,06
Cantidad disponible: 2 disponibles
Añadir al carritoHardcover. Condición: Brand New. 1st edition. 330 pages. 9.75x7.00x0.75 inches. In Stock.
Idioma: Inglés
Publicado por Cambridge University Press, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Librería: AHA-BUCH GmbH, Einbeck, Alemania
EUR 231,33
Cantidad disponible: 1 disponibles
Añadir al carritoBuch. Condición: 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.
Idioma: Inglés
Publicado por Cambridge University Press, Cambridge, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Librería: Grand Eagle Retail, Bensenville, IL, Estados Unidos de America
EUR 187,62
Cantidad disponible: 1 disponibles
Añadir al carritoHardcover. 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 multiple locations in the US or from the UK, depending on stock availability.
Librería: Revaluation Books, Exeter, Reino Unido
EUR 191,98
Cantidad disponible: 1 disponibles
Añadir al carritoHardcover. Condición: Brand New. 1st edition. 330 pages. 9.75x7.00x0.75 inches. In Stock. This item is printed on demand.
Idioma: Inglés
Publicado por Cambridge University Press, Cambridge, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Librería: CitiRetail, Stevenage, Reino Unido
EUR 195,25
Cantidad disponible: 1 disponibles
Añadir al carritoHardcover. 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. This item is printed on demand. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability.
Idioma: Inglés
Publicado por Cambridge University Press, 2016
ISBN 10: 0521855578 ISBN 13: 9780521855570
Librería: moluna, Greven, Alemania
EUR 186,71
Cantidad disponible: Más de 20 disponibles
Añadir al carritoGebunden. 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.
Idioma: Inglés
Publicado por Cambridge University Press, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Librería: THE SAINT BOOKSTORE, Southport, Reino Unido
EUR 231,85
Cantidad disponible: Más de 20 disponibles
Añadir al carritoHardback. Condición: New. This item is printed on demand. New copy - Usually dispatched within 5-9 working days.
Idioma: Inglés
Publicado por Cambridge University Press, Cambridge, 2006
ISBN 10: 0521855578 ISBN 13: 9780521855570
Librería: AussieBookSeller, Truganina, VIC, Australia
EUR 267,86
Cantidad disponible: 1 disponibles
Añadir al carritoHardcover. 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. This item is printed on demand. Shipping may be from our Sydney, NSW warehouse or from our UK or US warehouse, depending on stock availability.