國立高雄大學圖資館 |

Language: English

Back

Understanding the enrichment of heav...

Hirai, Yutaka.

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 galaxiesby Yutaka Hirai.
Author:	Hirai, Yutaka.
Published:	Singapore :Springer Singapore :2019.
Description:	xv, 135 p. :ill., digital ;24 cm.
Contained By:	Springer eBooks
Subject:	Dwarf galaxies.
Online resource:	https://doi.org/10.1007/978-981-13-7884-3
ISBN:	9789811378843$q(electronic bk.)

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$q(electronic bk.)

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

758844
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
LDR:02369nmm a2200349 a 4500 001 556939
003 DE-He213
005 20190430141552.0
006 m d
007 cr nn 008maaau
008 191127s2019 si s 0 eng d
020 $a 9789811378843$q(electronic bk.)
020 $a 9789811378836$q(paper)
023 3 3 $a nam a2200337 a 4500
024 7 $a 10.1007/978-981-13-7884-3 $2 doi
035 $a 978-981-13-7884-3
040 $a GP $c GP
041 0 $a eng
050 4 $a QB858 $b .H47 2019
072 7 $a PG $2 bicssc
072 7 $a SCI004000 $2 bisacsh
072 7 $a PG $2 thema
082 0 4 $a 523.112 $2 23
090 $a QB858 $b .H668 2019
100 1 $a Hirai, Yutaka. $3 839317
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 758844
650 0 $a Heavy elements. $3 814440
650 1 4 $a Astronomy, Observations and Techniques. $3 376735
650 2 4 $a Theoretical Astrophysics. $3 821426
650 2 4 $a Cosmology. $3 228629
650 2 4 $a Numerical and Computational Physics, Simulation. $3 758154
710 2 $a SpringerLink (Online service) $3 273601
773 0 $t Springer eBooks
830 0 $a Springer theses. $3 557607
856 4 0 $u https://doi.org/10.1007/978-981-13-7884-3
950 $a Physics and Astronomy (Springer-11651)