mcwilliam andrew rauch michael editors (2 risultati)

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.