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عنوان
Understanding the enrichment of heavy elements by the chemodynamical evolution models of dwarf galaxies /

پدید آورنده
Hirai Yutaka.

موضوع
Dwarf galaxies.,Heavy elements.,Dwarf galaxies.,Heavy elements.,SCIENCE-- Astronomy.

رده
QB858
.
H47
2019

کتابخانه
Center and Library of Islamic Studies in European Languages

محل استقرار
استان: Qom ـ شهر: Qom

Center and Library of Islamic Studies in European Languages

تماس با کتابخانه : 32910706-025

INTERNATIONAL STANDARD BOOK NUMBER

(Number (ISBN
9789811378843
(Number (ISBN
9789811378850
(Number (ISBN
9789811378867
(Number (ISBN
9811378843
(Number (ISBN
9811378851
(Number (ISBN
981137886X
Erroneous ISBN
9789811378836
Erroneous ISBN
9811378835

TITLE AND STATEMENT OF RESPONSIBILITY

Title Proper
Understanding the enrichment of heavy elements by the chemodynamical evolution models of dwarf galaxies /
General Material Designation
[Book]
First Statement of Responsibility
Hirai Yutaka.

.PUBLICATION, DISTRIBUTION, ETC

Place of Publication, Distribution, etc.
Singapore :
Name of Publisher, Distributor, etc.
Springer,
Date of Publication, Distribution, etc.
[2019]

PHYSICAL DESCRIPTION

Specific Material Designation and Extent of Item
1 online resource

SERIES

Series Title
Springer theses: recognizing outstanding Ph. D. research

GENERAL NOTES

Text of Note
Doctoral thesis accepted by the University of Tokyo, Tokyo, Japan.

INTERNAL BIBLIOGRAPHIES/INDEXES NOTE

Text of Note
Includes bibliographical references and index.

CONTENTS NOTE

Text of Note
Introduction -- Methods for simulations of galaxy formation -- Chemodynamical evolution of dwarf galaxies -- Enrichment of zinc in dwarf galaxies -- Enrichment of r-process elements in isolated dwarf galaxies -- Efficiency of metal mixing in dwarf galaxies -- Enrichment of r-process elements in a cosmological context -- Conclusions and future prospects.
0

SUMMARY OR ABSTRACT

Text of Note
This book addresses the mechanism of enrichment of heavy elements in galaxies, a long standing problem in astronomy. It mainly focuses on explaining the origin of heavy elements by performing state-of-the-art, high-resolution hydrodynamic simulations of dwarf galaxies. In this book, the author successfully develops a model of galactic chemodynamical evolution by means of which the neutron star mergers can be used to explain the observed abundance pattern of the heavy elements synthesized by the rapid neutron capture process, such as europium, gold, and uranium in the Local Group dwarf galaxies. The book argues that heavy elements are significant indicators of the evolutionary history of the early galaxies, and presents theoretical findings that open new avenues to understanding the formation and evolution of galaxies based on the abundance of heavy elements in metal-poor stars.

ACQUISITION INFORMATION NOTE

Source for Acquisition/Subscription Address
Springer Nature
Stock Number
com.springer.onix.9789811378843

OTHER EDITION IN ANOTHER MEDIUM

Title
Understanding the enrichment of heavy elements by the chemodynamical evolution models of dwarf galaxies.
International Standard Book Number
9789811378836

TOPICAL NAME USED AS SUBJECT

Dwarf galaxies.
Heavy elements.
Dwarf galaxies.
Heavy elements.
SCIENCE-- Astronomy.

(SUBJECT CATEGORY (Provisional

PG
PG
SCI-- 004000

DEWEY DECIMAL CLASSIFICATION

Number
523
.
112
Edition
23

LIBRARY OF CONGRESS CLASSIFICATION

Class number
QB858
Book number
.
H47
2019

PERSONAL NAME - PRIMARY RESPONSIBILITY

Hirai, Yutaka

ORIGINATING SOURCE

Date of Transaction
20200823230939.0
Cataloguing Rules (Descriptive Conventions))
pn

ELECTRONIC LOCATION AND ACCESS

Electronic name
 مطالعه متن کتاب 

[Book]

Y

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