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Chemical abundances and chemical evolution of the Magellanic Clouds: Prospects for the future

Published online by Cambridge University Press:  19 July 2016

M. A. Dopita
M. A. Dopita*
Affiliation:
Mt. Stromlo and Siding Spring Observatories, The Australian National University

Abstract

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The prospects for future advances in understanding the chemical evolution of the Magellanic Clouds is reviewed on the basis of results presented at IAU Symposium #148. These are divided into three areas, the metallicity - age relationships, the current abundance set, and the theory of the chemical evolution of the Clouds.

Type
Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 393 - 395
Copyright
Copyright © Kluwer 1991 

References

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