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.
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From the reviews
"... many excellent volumes on this subject have been written. In my opinion, this one is the best."
D.L. Faulkner in: Australian & New Zealand Physicist, 1995
"Will clearly be the standard text in the subject."
N.H. Baker, Columbia University
"Kippenhahn and Weigert's work compares favorably with the few similar works, many of which are now out of date. It is superior to some others in eschewing elegance of mathematical analysis in favor of a comprehensive understanding of the observed and deduced properties of stars, from their initial formation to their final collapse."
CHOICE
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.
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Versandziele, Kosten & DauerAnbieter: Antiquariat Bookfarm, Löbnitz, Deutschland
Softcover. Study edition, corr. 3rd print. 1994. XVI, 468 p. Ex-library with stamp and library-signature. GOOD condition, some traces of use. Ehem. Bibliotheksexemplar mit Signatur und Stempel. GUTER Zustand, ein paar Gebrauchsspuren. C-05500 3540580131 Sprache: Englisch Gewicht in Gramm: 550. Bestandsnummer des Verkäufers 2491754
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Paperback. Zustand: Very Good. No Jacket. May have limited writing in cover pages. Pages are unmarked. ~ ThriftBooks: Read More, Spend Less 1.55. Bestandsnummer des Verkäufers G3540580131I4N00
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Soft cover. Zustand: Very Good. Binding solid, pages clean and bright. Some shelf wear to covers. Bestandsnummer des Verkäufers HD005
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Soft cover. Zustand: 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. Bestandsnummer des Verkäufers 059950
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Originalbroschur. Zustand: Wie neu. CORRECTED 3. printing. 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. Bestandsnummer des Verkäufers 298315
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Zustand: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. 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 g. Bestandsnummer des Verkäufers 458674979
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Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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. Bestandsnummer des Verkäufers 9783540580133
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paperback. Zustand: New. In shrink wrap. Looks like an interesting title! Bestandsnummer des Verkäufers Q-3540580131
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