Sprache: Englisch
Verlag: Cambridge University Press, 1993
ISBN 10: 0521367107 ISBN 13: 9780521367103
Anbieter: ThriftBooks-Dallas, Dallas, TX, USA
Paperback. Zustand: Good. No Jacket. Pages can have notes/highlighting. Spine may show signs of wear. ~ ThriftBooks: Read More, Spend Less.
Sprache: Englisch
Verlag: Cambridge University Press, 1993
ISBN 10: 0521367107 ISBN 13: 9780521367103
Anbieter: WeBuyBooks, Rossendale, LANCS, Vereinigtes Königreich
EUR 2,50
Anzahl: 1 verfügbar
In den WarenkorbZustand: 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.
Sprache: Englisch
Verlag: Cambridge University Press, 1993
ISBN 10: 0521367107 ISBN 13: 9780521367103
Anbieter: Books From California, Simi Valley, CA, USA
Paperback. Zustand: Good.
Sprache: Englisch
Verlag: Cambridge University Press, 1993
ISBN 10: 0521367107 ISBN 13: 9780521367103
Anbieter: Better World Books Ltd, Dunfermline, Vereinigtes Königreich
EUR 5,39
Anzahl: 1 verfügbar
In den WarenkorbZustand: Good. Pages intact with minimal writing/highlighting. The binding may be loose and creased. Dust jackets/supplements are not included. Stock photo provided. Product includes identifying sticker. Better World Books: Buy Books. Do Good.
Sprache: Englisch
Verlag: Cambridge University Press, 1993
ISBN 10: 0521367107 ISBN 13: 9780521367103
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This book is a quantitative introduction to what is known or theorized about the structure and evolution of galactic systems. It begins with a general introduction to galaxies and a summary of our empirical observations of galaxies in the universe, including our own. There are then three chapters on galactic structure: the manner in which motions of stars determine galactic shape, the determination of galactic masses, and the structure of discs in spirals. Galactic evolution, especially changes in chemical composition over time, is then covered. The book concludes with a discussion of the origin of galaxies and their relation to more general questions in cosmology. The presentation is sufficiently mathematical so that quantitative results can be discussed in detail. Throughout, the author stresses what are currently accepted results and what theories may need revision in what continues to be a rapidly developing subject.