The attempt to understand the physics of the structure of stars and their change in time - their evolution - has been bothering many physicists and astronomers ever since the last century… Mehr…
The attempt to understand the physics of the structure of stars and their change in time - their evolution - has been bothering many physicists and astronomers ever since the last century. This long chain of successful research is well documented not only by numerous papers in the corresponding journals but also by a series of books. Some of them are so excellently written that despite their age they can still be recommended, and not only as documents of the state of the art at that time. A few outstanding examples are the books of R. Emden (1907), A. S. Eddington (1926), S. Chandrasekhar (1939), and M. Schwarzschild (1958). But our science has rapidly expanded in the last few decades, and new aspects have emerged which could not even be anticipated, say, 30 years ago and which today have to be carefully explored. This does not mean, however, that our ambition is to present a complete account of the latest and most refined numerical results. This can well be left to the large and growing number of excellent review articles. The present book is intended rather to be a textbook that will help students and teachers to understand these results as far as possible and present them in a simple and clear manner. We know how difficult this is since we ourselves have tried for the largest part of our scientific career to understand ""how the stars work"" - and then to make others believe it. | Stellar Structure and Evolution by Rudolf Kippenhahn Paperback | Indigo Chapters Books > Science & Nature > Space > Astronomy P10117, Rudolf Kippenhahn<
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Paperback, [PU: Springer-Verlag Berlin and Heidelberg GmbH & Co. KG], A complete and comprehensive treatment of the physics of the stellar interior and the underlying fundamental processe… Mehr…
Paperback, [PU: Springer-Verlag Berlin and Heidelberg GmbH & Co. KG], A complete and comprehensive treatment of the physics of the stellar interior and the underlying fundamental processes and parameters. The text presents an overview of the models developed to explain the stability, dynamics and evolution of the stars, and great care is taken to detail the various stages in a star's life., Astronomy, Space & Time, Astronomical Observation: Observatories, Equipment & Methods, Galaxies & Stars, Astrophysics<
Springer, 1994. Soft cover. Very Good. Very good, clean, tight copy. Text free of marks. Professional book dealer since 1999. All orders are processed promptly and carefully packaged wi… Mehr…
Springer, 1994. Soft cover. Very Good. Very good, clean, tight copy. Text free of marks. Professional book dealer since 1999. All orders are processed promptly and carefully packaged with tracking., Springer, 1994, 3<
The attempt to understand the physics of the structure of stars and their change in time - their evolution - has been bothering many physicists and astronomers ever since the last century… Mehr…
The attempt to understand the physics of the structure of stars and their change in time - their evolution - has been bothering many physicists and astronomers ever since the last century. This long chain of successful research is well documented not only by numerous papers in the corresponding journals but also by a series of books. Some of them are so excellently written that despite their age they can still be recommended, and not only as documents of the state of the art at that time. A few outstanding examples are the books of R. Emden (1907), A. S. Eddington (1926), S. Chandrasekhar (1939), and M. Schwarzschild (1958). But our science has rapidly expanded in the last few decades, and new aspects have emerged which could not even be anticipated, say, 30 years ago and which today have to be carefully explored. This does not mean, however, that our ambition is to present a complete account of the latest and most refined numerical results. This can well be left to the large and growing number of excellent review articles. The present book is intended rather to be a textbook that will help students and teachers to understand these results as far as possible and present them in a simple and clear manner. We know how difficult this is since we ourselves have tried for the largest part of our scientific career to understand ""how the stars work"" - and then to make others believe it. | Stellar Structure and Evolution by Rudolf Kippenhahn Paperback | Indigo Chapters Books > Science & Nature > Space > Astronomy P10117, Rudolf Kippenhahn<
Paperback, [PU: Springer-Verlag Berlin and Heidelberg GmbH & Co. KG], A complete and comprehensive treatment of the physics of the stellar interior and the underlying fundamental processe… Mehr…
Paperback, [PU: Springer-Verlag Berlin and Heidelberg GmbH & Co. KG], A complete and comprehensive treatment of the physics of the stellar interior and the underlying fundamental processes and parameters. The text presents an overview of the models developed to explain the stability, dynamics and evolution of the stars, and great care is taken to detail the various stages in a star's life., Astronomy, Space & Time, Astronomical Observation: Observatories, Equipment & Methods, Galaxies & Stars, Astrophysics<
Springer, 1994. Soft cover. Very Good. Very good, clean, tight copy. Text free of marks. Professional book dealer since 1999. All orders are processed promptly and carefully packaged wi… Mehr…
Springer, 1994. Soft cover. Very Good. Very good, clean, tight copy. Text free of marks. Professional book dealer since 1999. All orders are processed promptly and carefully packaged with tracking., Springer, 1994, 3<
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A complete and comprehensive treatment of the physics of the stellar interior and the underlying fundamental processes and parameters. The text presents an overview of the models developed to explain the stability, dynamics and evolution of the stars, and great care is taken to detail the various stages in a star's life. The authors have succeeded in producing a unique text based on their own pioneering work in stellar modeling.Since its publication, this textbook has come to be considered a classic by both readers and teachers in astrophysics. This study edition is intended for students in astronomy and physics alike.
Detailangaben zum Buch - Stellar Structure and Evolution
EAN (ISBN-13): 9783540580133 ISBN (ISBN-10): 3540580131 Gebundene Ausgabe Taschenbuch Erscheinungsjahr: 1994 Herausgeber: Springer Berlin 468 Seiten Gewicht: 0,701 kg Sprache: eng/Englisch
Buch in der Datenbank seit 2007-05-24T09:21:35+02:00 (Berlin) Detailseite zuletzt geändert am 2023-03-30T14:50:13+02:00 (Berlin) ISBN/EAN: 3540580131
ISBN - alternative Schreibweisen: 3-540-58013-1, 978-3-540-58013-3 Alternative Schreibweisen und verwandte Suchbegriffe: Autor des Buches: kipp, kippen, rudolf kippenhahn alfred weigert, eddington Titel des Buches: studienausgabe, evolution 911, evolution 101, stella, kippenhahn weigert, stellar structure and evolution astronomy and astrophysics library
Daten vom Verlag:
Autor/in: Rudolf Kippenhahn; Alfred Weigert Titel: Astronomy and Astrophysics Library; Stellar Structure and Evolution Verlag: Springer; Springer Berlin 468 Seiten Erscheinungsjahr: 1994-07-28 Berlin; Heidelberg; DE Sprache: Englisch 69,54 € (DE) 71,49 € (AT) 77,00 CHF (CH) Available XVI, 468 p. 7 illus.
I The Basic Equations.- 1. Coordinates, Mass Distribution, and Gravitational Field in Spherical Stars.- 2. Conservation of Momentum.- 3. The Virial Theorem.- 4. Conservation of Energy.- 5. Transport of Energy by Radiation and Conduction.- 6. Stability Against Local, Non-spherical Perturbations.- 7. Transport of Energy by Convection.- 8. The Chemical Composition.- II The Overall Problem.- 9. The Differential Equations of Stellar Evolution.- 10. Boundary Conditions.- 11. Numerical Procedure.- 12. Existence and Uniqueness of Solutions.- III Properties of Stellar Matter.- 13. The Ideal Gas with Radiation.- 14. Ionization.- 15. The Degenerate Electron Gas.- 16. The Equation of State of Stellar Matter.- 17. Opacity.- 18. Nuclear Energy Production.- IV Simple Stellar Models.- 19. Polytropic Gaseous Spheres.- 20. Homology Relations.- 21. Simple Models in the U-V Plane.- 22. The Main Sequence.- 23. Other Main Sequences.- 24. The Hayashi Line.- 25. Stability Considerations.- V Early Stellar Evolution.- 26. The Onset of Star Formation.- 27. The Formation of Protostars.- 28. Pre-Main-Sequence Contraction.- 29. From the Initial to the Present Sun.- 30. Chemical Evolution on the Main Sequence.- VI Post-Main-Sequence Evolution.- 31. Evolution Through Helium Burning — Massive Stars.- 32. Evolution Through Helium Burning — Low-Mass Stars.- 33. Later Phases.- 34. Final Explosions and Collapse.- VII Compact Objects.- 35. White Dwarfs.- 36. Neutron Stars.- 37. Black Holes.- VIII Pulsating Stars.- 38. Adiabatic Spherical Pulsations.- 39. Non-adiabatic Spherical Pulsations.- 40. Non-radial Stellar Oscillations.- IX Stellar Rotation.- 41. The Mechanics of Rotating Stellar Models.- 42. The Thermodynamics of Rotating Stellar Models.- 43. The Angular-Velocity Distribution in Stars.-References.
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