saul adelman (16 Ergebnisse)

Zustand: 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.

Broschiert; Zustand: Gut. 119 Seiten; Das hier angebotene Buch stammt aus einer teilaufgelösten Bibliothek und trägt die entsprechenden Kennzeichnungen (Rückenschild, Stempel.). Schnitt leicht staubschmutzig, ansonsten ordentlicher Erhaltungszustand; Sprache: Englisch Gewicht in Gramm: 300.

Zustand: Good. This is an ex-library book and may have the usual library/used-book markings inside.This book has soft covers. In good all round condition. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,600grams, ISBN:0130803820.

Hardcover. Zustand: Like New. First Edition. Firm, square and tight with sturdy hinges, just showing a few minor rubs and some mild cosmetic wear. Hence a non-text page is stamped 'damaged'. Despite such this book is in nearly new condition. Thus the contents are crisp, fresh and clean. Offered for sale at a very sensible price.

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.

Gr.-8°, original hardcover. 1. ed. With numerous images, VI, 200 p. Shelfmark on spine, stamp on title, otherwise fine copy. Sprache: Englisch Gewicht in Gramm: 0.

Zustand: New. In.

Gr.-8°, original hardcover. 1st ed. With numerous images, X, 313 p. Rare copy. Shelfmark, stamp on title, otherwise fine copy. Sprache: Englisch Gewicht in Gramm: 0.

Zustand: New. A review, first published in 1994, of studies of the 'hot stars' that comprise a halo around our Galaxy and similar stars in other galaxies. Editor(s): Adelman, Saul J.; Upgren, Arthur R.; Adelman, Carol J. Num Pages: 406 pages, black & white illustrations. BIC Classification: PGM; PHVB. Category: (P) Professional & Vocational. Dimension: 244 x 170 x 21. Weight in Grams: 650. . 2011. 1st Edition. paperback. . . . . Books ship from the US and Ireland.

Zustand: New. In.

Hardcover/ Pappband. Zustand: Gut. 200 S. Sehr guter Zustand ha1075073 Sprache: Englisch Gewicht in Gramm: 510.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - The stars that form a halo around our Galaxy are intriguing; they have abundances of elements that suggest they are old. The properties of these 'hot stars' and similar stars in other galaxies challenge the well-established theory of stellar evolution in many ways. Studying the collective properties of these stars provides important input to many areas of astrophysics - including the formation of our Galaxy, stellar evolution and the stellar populations of other galaxies. The study of hot stars in the halo of our Galaxy is undergoing an exciting renaissance owing to important new observations with the Hubble Space Telescope and ASTRO1 and to techniques recently developed for ground-based observations. Advances in computers have also recently led to a far more detailed and complete theoretical understanding of stellar evolution. This volume, first published in 1994, draws together the proceedings of a conference held in Union College, New York, which gathered experts in the field in question.

Zustand: New. A review, first published in 1994, of studies of the 'hot stars' that comprise a halo around our Galaxy and similar stars in other galaxies. Editor(s): Adelman, Saul J.; Upgren, Arthur R.; Adelman, Carol J. Num Pages: 406 pages, 150 b/w illus. BIC Classification: PGM; PHVB. Category: (P) Professional & Vocational. Dimension: 247 x 174 x 24. Weight in Grams: 914. . 1994. 1st Edition. hardcover. . . . . Books ship from the US and Ireland.

Hardcover. Zustand: Brand New. 386 pages. 10.00x7.00x1.00 inches. In Stock.

Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - The stars that form a halo around our Galaxy are intriguing; they have abundances of elements that suggest they are old. The properties of these 'hot stars' and similar stars in other galaxies challenge the well-established theory of stellar evolution in many ways. Studying the collective properties of these stars provides important input to many areas of astrophysics - including the formation of our Galaxy, stellar evolution and the stellar populations of other galaxies. The study of hot stars in the halo of our Galaxy is undergoing an exciting renaissance owing to important new observations with the Hubble Space Telescope and ASTRO1 and to techniques recently developed for ground-based observations. Advances in computers have also recently led to a far more detailed and complete theoretical understanding of stellar evolution. This volume, first published in 1994, draws together the proceedings of a conference held in Union College, New York, which gathered experts in the field in question.

Zustand: Minor rubbing. VG. orig.boards Minor rubbing. VG. 25x17cm, xxi,520 pp., Series: Proceedings of the International Astronomical Union Symposia and Colloquia Contents: Section A. Normal A-Stars; Section B. Stellar Evolution, Rotation, Binarity; Section C. Convection in Stars; Section D. Diffusion as the Mechanism of Element Segregation; Section E. Magnetic Fields; Section F. Chemically Peculiar Stars; Section G. Pulsating Variables; Section H. Evolved A-Type Stars; Section I. The A-Star Laboratory; Section J. Observational Challenges of A-Type Stars; Summary. ["Over the last few decades, nuclear processes, radiation transfer, opacities and many other important physical processes have been incorporated in the modelling of stars. As knowledge of these processes has advanced, it has become clear that other associated physical processes are not well understood. This volume investigates these processes, focusing on convection, diffusion, rotation, and magnetic fields. It is a valuable resource for researchers in the field of stellar astrophysics, and graduate students" - Publisher's description].