Sprache: Englisch
Verlag: Springer : Berlin, 03.1996., 1996
ISBN 10: 3540589635 ISBN 13: 9783540589631
Anbieter: Die Wortfreunde - Antiquariat Wirthwein Matthias Wirthwein, Mannheim, Deutschland
8°, OPp, gebundene Ausgabe. Auflage: 1996. 405 Seiten Einband mit leichten Lagerspuren, sonst sehr gut erhalten. Ungelesen. Sprache: Englisch Gewicht in Gramm: 742.
Hardcover. Corr. 3. printing. XIII, 392 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-05184 9783540589631 Sprache: Englisch Gewicht in Gramm: 550.
Anbieter: Ria Christie Collections, Uxbridge, Vereinigtes Königreich
EUR 103,15
Anzahl: Mehr als 20 verfügbar
In den WarenkorbZustand: New. In.
Sprache: Englisch
Verlag: Springer Berlin Heidelberg, Springer Berlin Heidelberg, 1996
ISBN 10: 3540589635 ISBN 13: 9783540589631
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Half a century ago, S. Chandrasekhar wrote these words in the preface to his l 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. [ . J 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).