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Understanding the enrichment of heav...

Hirai, Yutaka.

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

Record Type:	Electronic resources : Monograph/item
Title/Author:	Understanding the enrichment of heavy elements by the chemodynamical evolution models of dwarf galaxies/ by Yutaka Hirai.
Author:	Hirai, Yutaka.
Published:	Singapore :Springer Singapore : : 2019.,
Description:	xv, 135 p. :ill., digital ;24 cm.
[NT 15003449]:	Introduction -- Enrichment of r-Process Elements in Dwarf Spheroidal Galaxies in the Chemodynamical Evolution Models -- Early Chemodynamical Evolution of Dwarf Galaxies Deduced from r-Process Elements -- Enrichment of Zinc in Dwarf Galaxies -- Eﬃciency of Metal Mixing in Dwarf Galaxies -- Enrichment of r-Process Elements in a Cosmological Context -- Conclusions and Future Prospects.
Contained By:	Springer eBooks
Subject:	Dwarf galaxies. -
Online resource:	https://doi.org/10.1007/978-981-13-7884-3
ISBN:	9789811378843

Understanding the enrichment of heavy elements by the chemodynamical evolution models of dwarf galaxies
Hirai, Yutaka.

Understanding the enrichment of heavy elements by the chemodynamical evolution models of dwarf galaxies[electronic resource] /by Yutaka Hirai. - Singapore :Springer Singapore :2019. - xv, 135 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction -- Enrichment of r-Process Elements in Dwarf Spheroidal Galaxies in the Chemodynamical Evolution Models -- Early Chemodynamical Evolution of Dwarf Galaxies Deduced from r-Process Elements -- Enrichment of Zinc in Dwarf Galaxies -- Eﬃciency of Metal Mixing in Dwarf Galaxies -- Enrichment of r-Process Elements in a Cosmological Context -- Conclusions and Future Prospects.

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.

ISBN: 9789811378843

Standard No.: 10.1007/978-981-13-7884-3doiSubjects--Topical Terms:

2210506
Dwarf galaxies.

LC Class. No.: QB858 / .H47 2019

Dewey Class. No.: 523.112

Understanding the enrichment of heavy elements by the chemodynamical evolution models of dwarf galaxies
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100 1 $a Hirai, Yutaka. $3 3409332
245 1 0 $a Understanding the enrichment of heavy elements by the chemodynamical evolution models of dwarf galaxies $h [electronic resource] / $c by Yutaka Hirai.
260 $a Singapore : $b Springer Singapore : $b Imprint: Springer, $c 2019.
300 $a xv, 135 p. : $b ill., digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5053
505 0 $a Introduction -- Enrichment of r-Process Elements in Dwarf Spheroidal Galaxies in the Chemodynamical Evolution Models -- Early Chemodynamical Evolution of Dwarf Galaxies Deduced from r-Process Elements -- Enrichment of Zinc in Dwarf Galaxies -- Eﬃciency of Metal Mixing in Dwarf Galaxies -- Enrichment of r-Process Elements in a Cosmological Context -- Conclusions and Future Prospects.
520 $a 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.
650 0 $a Dwarf galaxies. $3 2210506
650 0 $a Heavy elements. $3 3320026
650 1 4 $a Astronomy, Observations and Techniques. $3 1066822
650 2 4 $a Theoretical Astrophysics. $3 3339055
650 2 4 $a Cosmology. $3 531904
650 2 4 $a Numerical and Computational Physics, Simulation. $3 2209853
710 2 $a SpringerLink (Online service) $3 836513
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830 0 $a Springer theses. $3 1314442
856 4 0 $u https://doi.org/10.1007/978-981-13-7884-3
950 $a Physics and Astronomy (Springer-11651)