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Structure and evolution of single and binary stars

Author: Camiel W H de Loore; C Doom
Publisher: Dordrecht ; Boston : Kluwer Academic Publishers, ©1992.
Series: Astrophysics and space science library, v. 179.
Edition/Format:   Print book : EnglishView all editions and formats
Summary:

New insights into the development of stellar interiors were obtained from studying stars in various stages of their lives, as well as with the help of fast computers, which gave a boost to the  Read more...

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Material Type: Internet resource
Document Type: Book, Internet Resource
All Authors / Contributors: Camiel W H de Loore; C Doom
ISBN: 0792317688 9780792317685
OCLC Number: 25711985
Description: xvi, 458 pages : illustrations ; 25 cm.
Contents: Foreword. 1. Introduction to the Stars. 2. The Equations of Stellar Structure. 3. The Equation of State. 4. Nuclear Reaction Rates. 5. Nuclear Burning in Stellar Interiors. 6. Astrophysical Opacities. 7. Stellar Convection. 8. Numerical Techniques. 9. The Formation of Stars. 10. Stellar Evolution During the Successive Nuclear Burning Phases. 11. The Evolution of Low Mass Stars. 12. The Evolution of Intermediate Stars (2.3-6M). 13. The Evolution of Massive Stars. 14. Final Stages of Single Star Evolution. 15. The Evolution of Binary Stars: General Considerations. 16. The Evolution of Low and Intermediate Mass Binaries. 17. The Evolution of Massive Close Binaries. 18. Final Stages of Close Binary Evolution. 19. Structure and Evolutionary Models for Single and Binary Stars. Annex: Polytropes. References. General References. Literature per Chapter. Subject Index.
Series Title: Astrophysics and space science library, v. 179.
Responsibility: C.W.H. De Loore and C. Doom.
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