Isbn: 9783540603559 - theory of orbits: perturbative and geometrical methods (astronomy and astrophysics library) (24 Ergebnisse)

Hardcover. Zustand: Very Good. None Issued. Volume two ONLY. Text is unmarked; pages are bright. Binding is sturdy. Covers are scuffed and worn around the edges. The corners of the covers are bumped and there are a couple dings on the edges of the front cover. No dust jacket, as issued. 432pp.

Hardcover. Zustand: Very Good ++. Hardcover. Very Good ++. Name at top of first page, otherwise in excellent condition.

hardcover. 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.…

Zustand: New. This is a Brand-new US Edition. This Item may be shipped from US or any other country as we have multiple locations worldwide.

Zustand: Brand New. New. US edition. Expediting shipping for all USA and Europe orders excluding PO Box. Excellent Customer Service.

Softcover. Zustand: Gut. [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. Zustand: Sehr gut. 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.

Zustand: Used. pp. 444.

Zustand: Used. pp. 444 52:B&W 6.14 x 9.21in or 234 x 156mm (Royal 8vo) Case Laminate on White w/Gloss Lam.

Zustand: Used. pp. 444.

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.

Zustand: New.

hardcover. Zustand: New. In shrink wrap. Looks like an interesting title.

hardcover. Zustand: New. In shrink wrap. Looks like an interesting title.

Zustand: New.

Zustand: As New. Unread book in perfect condition.

Zustand: New. In English.

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).…

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).…

Zustand: gut. 1998. Theory of Orbits: Perturbative and Geometrical Methods (Astronomy and Astrophysics Library) In deutscher Sprache. pages.

Buch. Zustand: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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). 440 pp. Englisch.…

Gebunden. Zustand: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Whilst the first volume treats the classical theory, this second one is the first book on stellar dynamics that presents modern chaos dynamics and its applications to astronomical problems to the studentsWhilst the first volume treats the classical t.…

Buch. Zustand: Neu. Theory of Orbits | Perturbative and Geometrical Methods | Dino Boccaletti (u. a.) | Buch | Astronomy and Astrophysics Library | xiv | Englisch | 1998 | Springer | EAN 9783540603559 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu Print on Demand. …

Buch. Zustand: Neu. This item is printed on demand - Print on Demand Titel. Neuware -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).Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 440 pp. Englisch.…