Verlag: Cambridge University Press, 1938
Anbieter: Anybook.com, Lincoln, Vereinigtes Königreich
EUR 27,54
Anzahl: 1 verfügbar
In den WarenkorbZustand: Poor. This is an ex-library book and may have the usual library/used-book markings inside.This book has hardback covers. In poor condition, suitable as a reading copy. No dust jacket. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,1150grams, ISBN:
26 x 18 cm. Original Leather. Zustand: Gut. 434 P. Blotchy and partly lightly rubbed and bumped. Contents: A Single Star-Drift./ The Solar Motion./ The Two Star-Streams./ The Ellipsoidal Theory./ Star Clusters./ Galactic Rotation, etc.; - With Figures. - Previous Owner Notice and Exlibris, Paper bronzy, a few red pencil underline and notice, cover hinge inside lightly broken, page edges lightly blotchy, otherwise in very good condition. English Language. deu B04-11-03Q Sprache: Deutsch Gewicht in Gramm: 444.
Verlag: Cambridge at the University Press, Cambridge, 1938
Anbieter: J. Wyatt Books, Ottawa, ON, Kanada
Erstausgabe
Hardcover. Zustand: Very Good. Zustand des Schutzumschlags: Very Good. First UK Edition. 434 pages with black and white diagrams throughout. Blue cloth covers with silver titles, top and base of spine and corners are very lightly worn, some light spotting on covers, endpapers and text edges are lightly yellowed, previous owner's name written on fpdep, otherwise text is unmarked, Very Good. White dust jacket with blue titles, not price clipped, spine is faded, top and base of spine, corners are lightly worn, with a few small chips, very small tear to middle of spine near front hinge, a few light spots, top edge lightly worn, Very Good. Book.
Verlag: University Press, 1938., Cambridge:, 1938
Anbieter: Jeff Weber Rare Books, Neuchatel, NEUCH, Schweiz
Erstausgabe
262 x 187 mm. 8vo. viii, 434 pp. 75 figs., 52 tables, index. Navy cloth, gilt spine; rear inner hinge neatly repaired. Ownership signature of Harold Levine on title. Very good. FIRST EDITION. Presents the subject of stellar dynamics in its full mathematical and observational development up to 1938.