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The Metal Pre-Enrichment of the Galactic Disk: Solving the G-Dwarf Problem

Published online by Cambridge University Press:  25 May 2016

M. Samland  and
G. Hensler
M. Samland
Affiliation:
Institut für Astronomie und Astrophysik, Universität Kiel, D-24098 Kiel, Germany
G. Hensler
Affiliation:
Institut für Astronomie und Astrophysik, Universität Kiel, D-24098 Kiel, Germany

Extract

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The stellar metallicity distribution of low-mass stars is one of the major touchstones for models describing the chemical evolution of our Galaxy. In contrast to the gaseous components, the abundances of the stellar components also reflect the temporal enrichment. Hence, the stellar metallicity distribution is a stringent test for evolutionary models of galaxies.

Type
Chapter 5: How Did the Milky Way Form?
Information
Symposium - International Astronomical Union , Volume 169: Unsolved Problems of the Milky Way , 1996 , pp. 395 - 401
Copyright
Copyright © Kluwer 1996 

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