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Titlebook: Chemical Evolution of Galaxies; Francesca Matteucci Book 2012 Springer-Verlag Berlin Heidelberg 2012 Chemical Evolution of Galaxies.Classi

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书目名称Chemical Evolution of Galaxies
编辑Francesca Matteucci
视频videohttp://file.papertrans.cn/225/224335/224335.mp4
概述Educates graduate students and young researchers to start their own research in the field.Outlines theoretical models of chemical evolution of galaxies and compares them with observational results.Tre
丛书名称Astronomy and Astrophysics Library
图书封面Titlebook: Chemical Evolution of Galaxies;  Francesca Matteucci Book 2012 Springer-Verlag Berlin Heidelberg 2012 Chemical Evolution of Galaxies.Classi
描述.The term “chemical evolution of galaxies” refers to the evolution of abundances of chemical species in galaxies, which is due to nuclear processes occurring in stars and to gas flows into and out of galaxies. .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 galaxies. The topic is approached in a didactical and logical manner via galaxy evolution models which are compared with observational results obtained in the last two decades: The reader is given an introduction to the concept of chemical abundances and learns about the main stellar populations in our Galaxy as well as about the classification of galaxy types and their main observables. In the core of the book, the construction and solution of chemical evolution models are discussed in detail, followed by descriptions and interpretations of observations of the chemical evolution of the Milky Way, spheroidal galaxies, irregular galaxies and of cosmic chemical evolution..The aim of this book is to provide an introduction to students
出版日期Book 2012
关键词Chemical Evolution of Galaxies; Classification of Galaxies; Galaxies; Nucleosynthesis in Stars; Star for
版次1
doihttps://doi.org/10.1007/978-3-642-22491-1
isbn_softcover978-3-642-43005-3
isbn_ebook978-3-642-22491-1Series ISSN 0941-7834 Series E-ISSN 2196-9698
issn_series 0941-7834
copyrightSpringer-Verlag Berlin Heidelberg 2012
The information of publication is updating

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Simple Models of Chemical Evolution,r the . (IRA), which states that all stars less massive than or equal to 1.. live forever, while all stars more massive than 1.. die instantaneously. This approximation is correct for stars below 1.. but it is incorrect for larger masses with lifetimes not negligible relative to the age of the Unive
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Chemical Evolution of Irregular Galaxies,nd rather simple objects with low metallicity and large gas content, suggesting that they are either young objects or have undergone discontinuous star formation activity (bursts) or a continuous but not efficient star formation. They are very interesting objects for studying galaxy evolution: in fa
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Francesca MatteucciEducates graduate students and young researchers to start their own research in the field.Outlines theoretical models of chemical evolution of galaxies and compares them with observational results.Tre
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