9783540603559 - Theory of Orbits: Perturbative and Geometrical Methods (Astronomy and Astrophysics Library) von Boccaletti, Dino; Pucacco, Giuseppe (7 Ergebnisse)

Zustand: Good. Most items will be dispatched the same or the next working day. A copy that has been read but remains in clean condition. All of the pages are intact and the cover is intact and the spine may show signs of wear. The book may have minor markings which are not specifically mentioned.

Softcover. [Corrected 2nd printing]. XIV, 422 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-05070 9783540603559 Sprache: Englisch Gewicht in Gramm: 1150.

8°, Pp., gebundene Ausgabe. XIV, 423 S. : graph. Darst. Einband mit leichten Lagerspuren, sonst sehr gut erhalten. Sieht kaum oder nicht gelesen aus. Sprache: Englisch Gewicht in Gramm: 765.

1st ed. 1999. 437 p. New! -- Neu und originalverschweißt! 9783540603559 Sprache: Englisch Gewicht in Gramm: 794 Hardcover: 15.6 x 2.7 x 23.4 cm.

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Zustand: Gut. Zustand: Gut | Seiten: 440 | Sprache: Englisch | Produktart: Bücher | Half a century ago, S. Chandrasekhar wrote these words in the preface to his 1 celebrated and successful book: In this monograph an attempt has been made to present the theory of stellar dy­ namics as a branch of classical dynamics - a discipline in the same general category as celestial mechanics. [ . ] Indeed, several of the problems of modern stellar dy­ namical theory are so severely classical that it is difficult to believe that they are not already discussed, for example, in Jacobi's Vorlesungen. Since then, stellar dynamics has developed in several directions and at var­ ious levels, basically three viewpoints remaining from which to look at the problems encountered in the interpretation of the phenomenology. Roughly speaking, we can say that a stellar system (cluster, galaxy, etc.) can be con­ sidered from the point of view of celestial mechanics (the N-body problem with N» 1), fluid mechanics (the system is represented by a material con­ tinuum), or statistical mechanics (one defines a distribution function for the positions and the states of motion of the components of the system).

Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Half a century ago, S. Chandrasekhar wrote these words in the preface to his 1 celebrated and successful book: In this monograph an attempt has been made to present the theory of stellar dy namics as a branch of classical dynamics - a discipline in the same general category as celestial mechanics. [ . ] Indeed, several of the problems of modern stellar dy namical theory are so severely classical that it is difficult to believe that they are not already discussed, for example, in Jacobi's Vorlesungen. Since then, stellar dynamics has developed in several directions and at var ious levels, basically three viewpoints remaining from which to look at the problems encountered in the interpretation of the phenomenology. Roughly speaking, we can say that a stellar system (cluster, galaxy, etc.) can be con sidered from the point of view of celestial mechanics (the N-body problem with N' 1), fluid mechanics (the system is represented by a material con tinuum), or statistical mechanics (one defines a distribution function for the positions and the states of motion of the components of the system).