Fr. 236.00

Evolutionary Processes in Binary Stars

English · Paperback / Softback

Shipping usually within 1 to 2 weeks (title will be printed to order)

Description

Read more

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 . . .

List of contents

1. Young Binary Stars; A.M. Ghez. 2. Observations of Discs Around Pre-Main-Sequence Binary Stars; R.D. Mathieu. 3. Dynamical Processes in Binary Star Formation; C. Clarke. 4. Young Binary Star/Disk Interactions; S.H. Lubow, P. Artymowicz. 5. Chaos and Tidal Capture; R.A. Mardling. 6. Hydrodynamic Encounters of Binaries; M.B. Davies. 7. Hydrodynamic Instabilities in Close Binary Systems; F.A. Rasio. 8. Common Envelope Evolution in Binary Systems; M. Livio. 9. Structure and Evolution of Massive Close Binaries; D. Vanbeveren. 10. Presupernova Evolution in Massive Binaries; Ph. Podsiadlowski, et al. 11. The Formation of Neutron Star and Black Hole Binaries; F. Verbunt. 12. Principles of Semi-Detached Binary Evolution; H. Ritter. 13. Magnetohydrodynamic Jets and Winds from Accretion Disks; H.C. Spruit. 14. Radiation Driven Evolution; F. D'Antona. 15. Binary Evolution of Type Ia Supernovae; J.C. Wheeler. 16. Black Holes in Binary Stars; R.A.M.J. Wijers. 17. Stellar and Dynamical Evolution within Triple Stars; P.P. Eggleton, L.G. Kiseleva. 18. Binary Population Synthesis: Theoretical Principles and an Example; M. de Kool. 19. An Observational Approach to Binary Population Synthesis; H.M. Johnston. Index. Object Index.

Product details

Assisted by Melvy B Davies (Editor), Melvyn B Davies (Editor), Melvyn B. Davies (Editor), Christopher Tout (Editor), Christopher A. Tout (Editor), R. A. Wijers (Editor), R.A. Wijers (Editor)
Publisher Springer Netherlands
 
Languages English
Product format Paperback / Softback
Released 25.07.2012
 
EAN 9789401072496
ISBN 978-94-0-107249-6
No. of pages 412
Illustrations XXVI, 412 p.
Series NATO Science Series C: (Closed
Nato Science Series C:
NATO Science Series C 177716
Nato Science Series C:
Subject Natural sciences, medicine, IT, technology > Physics, astronomy > Astronomy

Customer reviews

No reviews have been written for this item yet. Write the first review and be helpful to other users when they decide on a purchase.

Write a review

Thumbs up or thumbs down? Write your own review.

For messages to CeDe.ch please use the contact form.

The input fields marked * are obligatory

By submitting this form you agree to our data privacy statement.