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.
"Sinopsis" puede pertenecer a otra edición de este libro.
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"Kippenhahn and Weigert's work compares favorably with the few similar works, many of which are now out of date.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.
"Sobre este título" puede pertenecer a otra edición de este libro.
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Destinos, gastos y plazos de envíoLibrería: Antiquariat Bookfarm, Löbnitz, Alemania
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. Nº de ref. del artículo: 2491754
Cantidad disponible: 1 disponibles
Librería: The Secret Book and Record Store, Dublin, DUB, Irlanda
Soft cover. Condición: Very Good. Binding solid, pages clean and bright. Some shelf wear to covers. Nº de ref. del artículo: HD005
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Librería: 3rd St. Books, Lees Summit, MO, Estados Unidos de America
Soft cover. Condición: 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. Nº de ref. del artículo: 059950
Cantidad disponible: 1 disponibles
Librería: Chiemgauer Internet Antiquariat GbR, Altenmarkt, BAY, Alemania
Originalbroschur. Condición: Wie neu. CORRECTED 3. printing. XVI, 468 Seiten : graphische Darstellungen ; 25 cm FRISCHES, SEHR schönes Exemplar der KORRIGIERTEN Auflage. Sprache: Englisch Gewicht in Gramm: 700. Nº de ref. del artículo: 298315
Cantidad disponible: 1 disponibles
Librería: Ria Christie Collections, Uxbridge, Reino Unido
Condición: New. In. Nº de ref. del artículo: ria9783540580133_new
Cantidad disponible: Más de 20 disponibles
Librería: Chiron Media, Wallingford, Reino Unido
PF. Condición: New. Nº de ref. del artículo: 6666-IUK-9783540580133
Cantidad disponible: 10 disponibles
Librería: AHA-BUCH GmbH, Einbeck, Alemania
Taschenbuch. Condición: 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. Nº de ref. del artículo: 9783540580133
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Librería: moluna, Greven, Alemania
Condición: New. 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. Nº de ref. del artículo: 458674979
Cantidad disponible: Más de 20 disponibles
Librería: BennettBooksLtd, North Las Vegas, NV, Estados Unidos de America
paperback. Condición: New. In shrink wrap. Looks like an interesting title! Nº de ref. del artículo: Q-3540580131
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Librería: HPB-Red, Dallas, TX, Estados Unidos de America
Paperback. Condición: Good. Connecting readers with great books since 1972! Used textbooks may not include companion materials such as access codes, etc. May have some wear or writing/highlighting. We ship orders daily and Customer Service is our top priority! Nº de ref. del artículo: S_425267189
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