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The interstellar medium of the Magellanic Clouds from absorption lines

Published online by Cambridge University Press:  19 July 2016

Klaas S. De Boer
Klaas S. De Boer*
Affiliation:
Sternwarte, University of Bonn, Auf dem Hügel 71, D-5300 Bonn, F.R. Germany

Abstract

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General aspects of ISM studies using absorption line studies are given and available data are reviewed. Topics are: galactic foreground gas, individual fields in the Magellanic Clouds (MCs) and MC coronae. Overall investigations are discussed. It is demonstrated that the metals in the gas of the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC) are a factor of 3 and 10, respectively, in abundance below solar levels. The depletion pattern in the LMC is similar to that of the Milky Way.

Type
The Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 401 - 406
Copyright
Copyright © Kluwer 1991 

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