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Molecular Line Observations in the Magellanic Clouds

Published online by Cambridge University Press:  30 March 2016

Mónica Rubio
Mónica Rubio*
Affiliation:
Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago, Chile

Abstract

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We review the present knowledge of molecular line studies and its relation to interstellar medium properties in the Large and Small Magellanic Clouds. The physical and chemical properties of the molecular gas together with the abundance of different molecular species will be discussed.

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 854 - 859
Copyright
Copyright © Astronomical Society of Pacific 2005

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