Evolutionary Processes Binary Stars (79 results)

Condition: New.

Condition: 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. . . . . …

Condition: New. In English.

Condition: New. pp. 332.

Condition: 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. Condition: 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.

Taschenbuch. Condition: 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. …

Condition: As New. Unread book in perfect condition.

Condition: New.

Condition: New.

Condition: 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. . . . . …

Condition: New.

Condition: New.

Condition: New. In English.

Condition: New.

Condition: As New. Unread book in perfect condition.

Hardback. Condition: 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. …

Condition: New. Proceedings of the NATO Advanced Study Institute, Cambridge, United Kingdom, July 10-21, 1995 7 Hydrodynamic Instabilities in Close Binary Systems (Frederic A. Rasio) 121 7. 1 Introduction. . . . . . . . . . . . . . . . . . . . . . . . 121 7. 1. 1 The .

Condition: New.

Condition: New.

Buch. Condition: Neu. Evolutionary Processes in Binary Stars | R. A. Wijers (u. a.) | Buch | Nato Science Series C: | Einband - fest (Hardcover) | Englisch | 1996 | Springer Netherlands | EAN 9780792340041 | Verantwortliche Person für die EU: Springer Nature Customer Service Center GmbH, Europaplatz 3, 69115 Heidelberg, productsafety[at]springernature[dot]com | Anbieter: preigu.…

Condition: 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 6-10 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.…

Condition: New. In English.

Condition: New. In English.

Condition: 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. . . . . …

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

Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - 7 Hydrodynamic Instabilities in Close Binary Systems (Frederic A. Rasio) 121 7. 1 Introduction. . . . . . . . . . . . . . . . . . . . . . . . 121 7. 1. 1 The stability of self-gravitating fluid equilibria 121 7. 1. 2 Astrophysical motivation . 123 7. 1. 3 Common envelope systems 125 7. 2 Dynamical instabilities. . . . . . . 126 7. 2. 1 Physical mechanism . . . . 126 7. 2. 2 Application to coalescing neutron star binaries 127 7. 3 Secular instabilities. . . . . . . . . . . 130 7. 3. 1 Physical mechanism . . . . . . 130 7. 3. 2 Application to contact binaries 133 8 Common Envelope Evolution in Binary Systems (Mario Livio) 141 8. 1 Introduction. . . . . . . . . . . . . . . . . . . . 141 8. 2 The entrance into the common envelope phase . . . . . 142 8. 3 The outcome of the CE phase. . . . . . . . . . . . . . . 145 8. 4 How close can we get to observing the common envelope Phase . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 146 8. 4. 1 How can PNe with binary nuclei be used to constrain CE physics . . . . . . . . . . . . . . . . . . . . . . . . . . . 147 8. 4. 2 How can nova systems be used to constrain CE physics 148 8. 4. 3 Other tests of common envelope evolution 150 8. 5 Conclusions . . . . . . . . . . . . . . . . . . . . . . . 151 9 Structure and Evolution of Massive Close Binaries (Dany Vanbeveren) 155 9. 1 Introduction. . . . . . . . . . . . . . . . . . 155 9. 2 Definitions. . . . . . . . . . . . . . . . . . . 156 9. 3 Intermediate mass and massive single stars 156 9. 3. 1 Observations . . . . . . . . . . . . . 156 9. 3. 2 Stellar structure equations for non-rotating IMS's and MS's 160 9. 3. 3 Evolutionary computations of non-rotating IMS's and MS's 162 9. 3. 4 Overall comparison with observations '' 163 9. 3. 5 The role of rotation in single star evolution . . .…

Buch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - 7 Hydrodynamic Instabilities in Close Binary Systems (Frederic A. Rasio) 121 7. 1 Introduction. . . . . . . . . . . . . . . . . . . . . . . . 121 7. 1. 1 The stability of self-gravitating fluid equilibria 121 7. 1. 2 Astrophysical motivation . 123 7. 1. 3 Common envelope systems 125 7. 2 Dynamical instabilities. . . . . . . 126 7. 2. 1 Physical mechanism . . . . 126 7. 2. 2 Application to coalescing neutron star binaries 127 7. 3 Secular instabilities. . . . . . . . . . . 130 7. 3. 1 Physical mechanism . . . . . . 130 7. 3. 2 Application to contact binaries 133 8 Common Envelope Evolution in Binary Systems (Mario Livio) 141 8. 1 Introduction. . . . . . . . . . . . . . . . . . . . 141 8. 2 The entrance into the common envelope phase . . . . . 142 8. 3 The outcome of the CE phase. . . . . . . . . . . . . . . 145 8. 4 How close can we get to observing the common envelope Phase . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 146 8. 4. 1 How can PNe with binary nuclei be used to constrain CE physics . . . . . . . . . . . . . . . . . . . . . . . . . . . 147 8. 4. 2 How can nova systems be used to constrain CE physics 148 8. 4. 3 Other tests of common envelope evolution 150 8. 5 Conclusions . . . . . . . . . . . . . . . . . . . . . . . 151 9 Structure and Evolution of Massive Close Binaries (Dany Vanbeveren) 155 9. 1 Introduction. . . . . . . . . . . . . . . . . . 155 9. 2 Definitions. . . . . . . . . . . . . . . . . . . 156 9. 3 Intermediate mass and massive single stars 156 9. 3. 1 Observations . . . . . . . . . . . . . 156 9. 3. 2 Stellar structure equations for non-rotating IMS's and MS's 160 9. 3. 3 Evolutionary computations of non-rotating IMS's and MS's 162 9. 3. 4 Overall comparison with observations '' 163 9. 3. 5 The role of rotation in single star evolution . . .…

Buch. Condition: 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.…