Andrew mcwilliam michael rauch (39 risultati)

Condizione: New.

Condizione: New.

Condizione: As New. Unread book in perfect condition.

Condizione: New.

Condizione: New. This Carnegie volume discusses the origin and evolution of elements in our galaxy and others. Editor(s): McWilliam, Andrew; Rauch, Michael. Num Pages: 514 pages, 184 b/w illus. 24 tables. BIC Classification: PHVB. Category: (UP) Postgraduate, Research & Scholarly. Dimension: 245 x 172 x 24. Weight in Grams: 884. . 2010. Reissue. paperback. . . . .…

Condizione: As New. Unread book in perfect condition.

Condizione: New. This Carnegie volume discusses the origin and evolution of elements in our galaxy and others. Editor(s): McWilliam, Andrew; Rauch, Michael. Num Pages: 514 pages, 184 b/w illus. 24 tables. BIC Classification: PHVB. Category: (UP) Postgraduate, Research & Scholarly. Dimension: 245 x 172 x 24. Weight in Grams: 884. . 2010. Reissue. paperback. . . . . Books ship from the US and Ireland.…

Taschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - This comprehensive volume reviews our understanding of the origin and evolution of elements, from stellar nucleosynthesis to the chemical evolution of the cosmos. With chapters by leading authorities in the field, it describes models of how the elements are produced by stars, the nuclear processes involved, and how the quantity of elements evolved in our Galaxy and distant galaxies. The observed chemical composition of stars in different locations within our Galaxy and nearby galaxies is discussed, as are the compositions of hot and cold gases, of dust grains found between stars and in meteorites, and of the integrated light from distant galaxies and quasars. This authoritative volume is a valuable resource for graduate students and professional research astronomers.…

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

Condizione: New.

Condizione: New. pp. xvi + 496.

Condizione: New. pp. xvi + 496 Illus.

Hardcover. Condizione: Gut. Ehem. Bibliotheksexemplar mit Signatur und Stempel. GUTER Zustand, ein paar Gebrauchsspuren. Ex-library with stamp and library-signature. GOOD condition, some traces of use. D03845 9780521755788 Sprache: Englisch Gewicht in Gramm: 1150.

Condizione: New. pp. xvi + 496.

Condizione: New.

Condizione: New.

Condizione: New. This Carnegie volume discusses the origin and evolution of elements in our galaxy and others. Editor(s): McWilliam, Andrew; Rauch, Michael. Num Pages: 514 pages, 184 b/w illus. 24 tables. BIC Classification: PHVB. Category: (P) Professional & Vocational. Dimension: 247 x 174 x 29. Weight in Grams: 1205. . 2004. Illustrated. hardcover. . . . . …

Hardback. Condizione: New. This comprehensive volume reviews our understanding of the origin and evolution of elements, from stellar nucleosynthesis to the chemical evolution of the cosmos. With chapters by leading authorities in the field, it describes models of how the elements are produced by stars, the nuclear processes involved, and how the quantity of elements evolved in our Galaxy and distant galaxies. The observed chemical composition of stars in different locations within our Galaxy and nearby galaxies is discussed, as are the compositions of hot and cold gases, of dust grains found between stars and in meteorites, and of the integrated light from distant galaxies and quasars. This authoritative volume is a valuable resource for graduate students and professional research astronomers.…

Condizione: As New. Unread book in perfect condition.

Hardcover. Condizione: Like New. LIKE NEW. SHIPS FROM MULTIPLE LOCATIONS. book.

Condizione: New. This Carnegie volume discusses the origin and evolution of elements in our galaxy and others. Editor(s): McWilliam, Andrew; Rauch, Michael. Num Pages: 514 pages, 184 b/w illus. 24 tables. BIC Classification: PHVB. Category: (P) Professional & Vocational. Dimension: 247 x 174 x 29. Weight in Grams: 1205. . 2004. Illustrated. hardcover. . . . . Books ship from the US and Ireland. …

Condizione: As New. Unread book in perfect condition.

Hardcover. Condizione: Brand New. 496 pages. 9.75x7.00x1.00 inches. In Stock.

Buch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - This comprehensive volume reviews our understanding of the origin and evolution of elements, from stellar nucleosynthesis to the chemical evolution of the cosmos. With chapters by leading authorities in the field, it describes models of how the elements are produced by stars, the nuclear processes involved, and how the quantity of elements evolved in our Galaxy and distant galaxies. The observed chemical composition of stars in different locations within our Galaxy and nearby galaxies is discussed, as are the compositions of hot and cold gases, of dust grains found between stars and in meteorites, and of the integrated light from distant galaxies and quasars. This authoritative volume is a valuable resource for graduate students and professional research astronomers.…

Hardback. Condizione: New. This comprehensive volume reviews our understanding of the origin and evolution of elements, from stellar nucleosynthesis to the chemical evolution of the cosmos. With chapters by leading authorities in the field, it describes models of how the elements are produced by stars, the nuclear processes involved, and how the quantity of elements evolved in our Galaxy and distant galaxies. The observed chemical composition of stars in different locations within our Galaxy and nearby galaxies is discussed, as are the compositions of hot and cold gases, of dust grains found between stars and in meteorites, and of the integrated light from distant galaxies and quasars. This authoritative volume is a valuable resource for graduate students and professional research astronomers.…

orig.boards Some rubbing. Binding corner bumps. VG. Textual graphs,photos,charts 25x17cm, xvi,496 pp, Series: Carnegie Symposium on Origin and Evolution of the Elements/ Carnegie Observatories Astrophysics Series. Contains 31 papers. Includes: Mount Wilson Observatory Contributions to the Study of Cosmic Abundances of the Chemical Elements; Synthesis of the Elements in Stars: B2-FH & Beyond; Stellar Nucleosynthesis: A Status Report 2003; Advances in R-Process Nucleosynthesis; Element Yields of Intermediate-Mass Stars; The Impact of Rotation on Chemical Abundances in Red Giant Branch Stars; S-Processing in AGB Stars & the Composition of Carbon Stars; Models of Chemical Evolution; Model Atmospheres & Stellar Abundance Analysis; The Light Elements. Lithium, Beryllium & Boron; Extremely Metal-Poor Stars; Thin & Thick Galactic Disks; Globular Clusters & Halo Field Stars; Chemical Evolution in W-Centauri; Chemical Composition of the Magellanic Clouds, From Young to Old Stars; Detailed Composition of Stars in Dwarf Spheroid Galaxies; The Evolutionary History of Local Group Irregular Galaxies; Chemcial Evolution of the Old Stellar Populations of M31; Stellar Winds of Hot Massive Stars Nearby & Beyond the Local Group; Presolar Stardust Grains; Interstellar Dust; Interstellar Atomic Abundances; Molecules in the Interstellar Medium; Metal Ejection by Galactic Winds; Abundances from the Integrated Light of Globular Clusters &Galaxies; Abundances in Spiral & Irregular Galaxies; Chemical Compositoon of the Intracluster Medium; Quasar Elemental Abundances & Host Galaxy Evolution; Chemical Abundances in the Damped Lya Systems; Intergalactic Medium Abundances. Some rubbing. Binding corner bumps. VG.…

orig.boards Minor rubbing. An ink mark to top page-edge. VG. 25x17cm, xvi,496 pp., Series: Carnegie Observatories Astrophysics Series, vol. 4. "This 2004 comprehensive volume reviews our understanding of the origin and evolution of elements, from stellar nucleosynthesis to the chemical evolution of the cosmos. With chapters by leading authorities in the field,it describes models of how the elements are produced by stars, the nuclear processes involved, and how the quantity of elements evolved in our Galaxy and distant galaxies. The observed chemical composition of stars in different locations within our Galaxy and nearby galaxies is discussed, as are the compositions of hot and cold gases, of dust grains found between stars and in meteorites, and of the integrated light from distant galaxies and quasars. This authoritative volume is a valuable resource for graduate students and professional research astronomers" - publisher's description. Minor rubbing. An ink mark to top page-edge. VG.…

PF. Condizione: New. This item is printed on demand. Brand new book, sourced directly from publisher. Dispatch time is 6-7 days from our warehouse. Book will be sent in robust, secure packaging to ensure it reaches you securely.

Condizione: New. Print on Demand pp. 514 67:B&W 6.69 x 9.61 in or 244 x 170 mm (Pinched Crown) Perfect Bound on White w/Gloss Lam.

Condizione: New. Print on Demand pp. 514.