Übersicht			Auf mobile öffnen

Lieferstatus:	Auf Bestellung (Lieferzeit unbekannt)
Veröffentlichung:	Mai 2019
Genre:	Naturwissensch., Medizin, Technik
	Astronomy, Cosmology and Space Sciences / Astronomy, Observations and Techniques / Astronomy—Observations / Astrophysics / B / Cosmology / Mathematical physics / Numerical and Computational Physics, Simulation / Observations, Astronomical / Physics / Physics and Astronomy / Relativity physics / Theoretical & mathematical astronomy / Theoretical Astrophysics / Theoretical, Mathematical and Computational Physics
ISBN:	9789811378836
EAN-Code:	9789811378836
Verlag:	Springer Nature EN
Einband:	Gebunden
Sprache:	English
Serie:	Springer Theses
Dimensionen:	H 235 mm / B 155 mm / D
Gewicht:	401 gr
Seiten:	135
Illustration:	XV, 135 p. 70 illus., 66 illus. in color., schwarz-weiss Illustrationen, farbige Illustrationen
Bewertung:	Titel bewerten / Meinung schreiben

Inhalt:

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.