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Multi-wavelength View of the Interstellar Medium in the Large Magellanic Cloud

Published online by Cambridge University Press:  16 May 2016

You-Hua Chu
You-Hua Chu*
Affiliation:
Department of Astronomy, University of Illinois, 1002 W. Green Street, Urbana, IL 61801, USA; chu@astro.uiuc.edu
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Abstract

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The Large Magellanic Cloud (LMC) has been surveyed in optical emission lines, X-rays, radio continuum, HI, and CO lines. These surveys provide views of the interstellar medium (ISM) in the LMC of unprecedented clarity, allowing us to study astrophysical processes and to examine the relationship among the different phases of the ISM. Multi-wavelength images are used to illustrate the physical structures of supernova remnants, superbubbles, and supergiant shells, as well as the global interstellar structure of the LMC.

Keywords

Magellanic Cloudsgalaxies: ISMISM: generalISM: structureISM: bubblessupernova remnants
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 15 , Issue 1 , 1998 , pp. 136 - 140
Copyright
Copyright © Astronomical Society of Australia 1998

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