Articles liés à Chemical Evolution of Galaxies
Chemical Evolution of Galaxies - Couverture souple
Livre 17 sur 55: Astronomy and Astrophysics Library
Synopsis
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 as well as to amend our present ideas in research; the book also summarizes the efforts made by authors in the past several years in order to further future research in the field.
Les informations fournies dans la section « Synopsis » peuvent faire référence à une autre édition de ce titre.
À propos de l'auteur
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.
Les informations fournies dans la section « A propos du livre » peuvent faire référence à une autre édition de ce titre.
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Chemical Evolution of Galaxies (eng)
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Chemical Evolution of Galaxies
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Berlin Springer Berlin Heidelberg Springer Feb 2014, 2014
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ISBN 13 : 9783642430053
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Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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 as well as to amend our present ideas in research; the book also summarizes the efforts made by authors in the past several years in order to further future research in the field. 226 pp. Englisch. N° de réf. du vendeur 9783642430053
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Chemical Evolution of Galaxies
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Springer Berlin Heidelberg, 2014
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Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. 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 Treats all main aspects of chemical evoluti. N° de réf. du vendeur 5060540
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Taschenbuch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - 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 as well as to amend our present ideas in research; the book also summarizes the efforts made by authors in the past several years in order to further future research in the field. N° de réf. du vendeur 9783642430053
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Chemical Evolution of Galaxies
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Springer, J.B. Metzler Feb 2014, 2014
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Taschenbuch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -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 adidactical 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 modelsare 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 as well as toamend our present ideas in research; the book also summarizes the efforts made by authors in the past several years in order tofurther future research in the field.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 240 pp. Englisch. N° de réf. du vendeur 9783642430053
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