Stellar structure and evolution.

Kippenhahn, Rudolf and Alfred Weigert:

ISBN 10: 3540580131 / ISBN 13: 9783540580133

Edité par Berlin ; Heidelberg ; New York ; London ; Paris ; Tokyo ; Hong Kong ; Barcelona ; Budapest : Springer, 1994

A propos de cet article

XVI, 468 Seiten : graphische Darstellungen ; 25 cm FRISCHES, SEHR schönes Exemplar der KORRIGIERTEN Auflage. ( we have a lot of books on PHYSICS and MATHEMATICS on stock in EXCELLENT shape) Sprache: Englisch Gewicht in Gramm: 700.

N° de réf. du vendeur 298315

Détails bibliographiques

• Titre: Stellar structure and evolution.
• Éditeur: Berlin ; Heidelberg ; New York ; London ; Paris ; Tokyo ; Hong Kong ; Barcelona ; Budapest : Springer
• Date de parution: 1994
• Langue: anglais
• ISBN à 10 chiffres: 3540580131
• ISBN à 13 chiffres: 9783540580133
• Reliure: Originalbroschur.
• Édition: CORRECTED 3. printing.
• État de l'article: Wie neu
• Catalogues du vendeur:
  • Astronomie

A propos de ce titre

Synopsis

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.