This book is based partly on a. lecture course given at the University of Tri este, but mostly on my own research experience in the field of galactic chemical evolution. The subject of galactic chemical evolution was started and developed by Beat rice Tinsley in the seventies and now is a flourishing subject. This book is dedi cated to the chemical evolution of our Galaxy and aims at giving an up-to-date review of what we have learned since Tinsley's pioneering efforts. At the time of writing, in fact, books of this kind were not available with the exception of the excellent book by Bernard Pagel on "Nucleosynthesis and Chemical Evolution of Galaxies" (Cambridge University Press, 1997), and the subject of galactic chem ical evolution has appeared only as short chapters in books devoted to other subjects. Therefore, I felt that a book of this kind could be useful. The book summarizes the observational facts which allow us to reconstruct the chemical history of our Galaxy, in particular the abundances in stars and in terstellar medium; in the last decade, a great deal of observational work, mostly abundance determinations in stars in the solar vicinity, has shed light on the pro duction and distribution of chemical elements. Even more recently more abun dance data have accumulated for external galaxies at both low and high redshift, thus providing precious information on the chemical evolution of different types of galaxies and on the early stages of galaxy evolution.
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Joss Bland-Hawthorn holds the Federation Fellow Professorship at the Institute of Astronomy, School of Physics, University of Sydney. He is doing research on near-field and far-field cosmology and is also working in instrument science. Kenneth Charles Freeman is Duffield Professor of Astronomy in the Research School of Astronomy and Astrophysics at the Mount Stromlo Observatory of the Australian National University in Canberra. His research interests are in the formation and dynamics of galaxies and globular clusters. He received several international awards. Francesca Matteucci is associate professor at the University of Trieste, Italy, where she teaches Stellar Physics. Her field of research is the chemical evolution of galaxies of different morphological type, supernova rates and supernova progenitors.
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Zustand: New. Provides a discussion of the evolution of elemental abundances in the Galaxy taking into account both spatial and temporal variations. This work interprets the observed chemical abundances in terms of formation and evolution of the Galaxy. It is useful for scientists and graduate students. Series: Astrophysics and Space Science Library. Num Pages: 299 pages, biography. BIC Classification: PG. Category: (P) Professional & Vocational. Dimension: 240 x 160 x 16. Weight in Grams: 532. . 2003. Softcover reprint of the original 1st ed. 2003. Paperback. . . . . Books ship from the US and Ireland. Artikel-Nr. V9781402016523
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Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This book is based partly on a. lecture course given at the University of Tri este, but mostly on my own research experience in the field of galactic chemical evolution. The subject of galactic chemical evolution was started and developed by Beat rice Tinsley in the seventies and now is a flourishing subject. This book is dedi cated to the chemical evolution of our Galaxy and aims at giving an up-to-date review of what we have learned since Tinsley's pioneering efforts. At the time of writing, in fact, books of this kind were not available with the exception of the excellent book by Bernard Pagel on 'Nucleosynthesis and Chemical Evolution of Galaxies' (Cambridge University Press, 1997), and the subject of galactic chem ical evolution has appeared only as short chapters in books devoted to other subjects. Therefore, I felt that a book of this kind could be useful. The book summarizes the observational facts which allow us to reconstruct the chemical history of our Galaxy, in particular the abundances in stars and in terstellar medium; in the last decade, a great deal of observational work, mostly abundance determinations in stars in the solar vicinity, has shed light on the pro duction and distribution of chemical elements. Even more recently more abun dance data have accumulated for external galaxies at both low and high redshift, thus providing precious information on the chemical evolution of different types of galaxies and on the early stages of galaxy evolution. Artikel-Nr. 9781402016523
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