Includes bibliographical references (p. 277-292).
|Statement||by Francesca Matteucci.|
|Series||Astrophysics and space science library -- v. 253.|
|LC Classifications||QB857.7 .M38 2001, QB857.7 .M38 2001|
|The Physical Object|
|Pagination||xii, 293 p. :|
|Number of Pages||293|
|LC Control Number||00060503|
From the reviews: “In order to evolve a galaxy, you must choose a mass of gas; decide on a prescription for turning it into stars . Matteucci’s book explains how to do all these things, ending with a discussion of cosmic chemical evolution . anyone wanting to get up to speed quickly on the topic should find the book very by: 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 . Preface. 1. Observational Evidence for Chemical Evolution. 2. Stellar Evolution and Nucleosynthesis. 3. The Stellar Birthrate. 4. Gas Flows. 5. Basic Equations of Chemical Evolution. 6. Formation and Evolution of the Milky Way. 7. Nucleochronology and the Age of the Galaxy. 8. The Milky Way and Other Spiral Galaxies. Series Title. Download The Chemical Evolution Of The Galaxy Book For Free in PDF, EPUB. In order to read online The Chemical Evolution Of The Galaxy textbook, you need to create a FREE account. Read as many books as you like (Personal use) and Join Over Happy Readers. We cannot guarantee that every book is in the library.
Chemical abundances provide important clues to the evolution of galaxies. Ionized nebulae are one of the main sources of chemical abundance measurements, especially in external galaxies. Studies of H I regions have shown that the overall metallicity of galaxies increases with galactic luminosity, and . This volume provides a thorough discussion of the evolution of elemental abundances in the Galaxy taking into account both spatial and temporal variations. For the first time, and in much greater detail, the observed chemical abundances are interpreted in terms of formation and evolution of the Galaxy. Observational constraints like the gas and star formation rate distribution are guiding this Cited by: This book is devoted to the study of the evolution of the abundances of the chemical elements both in time and space in our own Galaxy. The new aspects of this book consist in the interpretation of the chemical abundances and other observational constraints (e.g., gas and star formation rate distribution) in terms of the formation and evolution of the Milky Way. • This implies that the chemical abundance of the gas in a galaxy should evolve in time. If there is no gas infall from the outside, then the metal abundance of the gas, and hence of the stars, should increase in time. • Therefore, the evolution of chemical element abundances in a galaxy .
ISBN: OCLC Number: Description: 1 online resource ( pages) Contents: 1. Observational Evidence for Chemical Evolution Overview and historical perspective Abundances in stars Abundances in globular clusters The metallicity distribution of the local disk G-dwarfs The metallicity distribution of halo. This book deals with the chemical evolution of galaxies of all morphological types (ellipticals, spirals and irregulars) and stresses the importance of the star formation histories in determining the properties of stellar populations in different : Springer-Verlag Berlin Heidelberg. Download The Chemical Evolution Of The Galaxy full book in PDF, EPUB, and Mobi Format, get it for read on your Kindle device, PC, phones or tablets. The Chemical Evolution Of The Galaxy full free pdf books. Abstract. Over the last few years, our picture of the chemical evolution of the Galaxy has changed substantially. These changes are of interest because chemical evolution provides a common point of contact for most astrophysical processes of importance to galaxy evolution.