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The violent interstellar medium of the Magellanic Cloud System

Published online by Cambridge University Press:  01 July 2008

You-Hua Chu
You-Hua Chu*
Affiliation:
Astronomy Department, University of Illinois, 1002 W. Green Street, Urbana, IL 61801, USA email: [email protected]
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Abstract

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The interstellar gas of the Magellanic System is subject to the harassment of tidal interactions on galaxy-wide scales and stellar energy feedback on sub-galactic scales. H i surveys of the Magellanic System have produced spectacular images of the tidally displaced interstellar gas in the Magellanic Bridge and Streams. Multi-wavelength observations of the interstellar gas in the Magellanic Clouds have revealed gas components in physical conditions ranging from cold molecular cloud to hot ionized coronal gas. While stellar energy feedback is responsible for heating and dispersing interstellar gas, it can also compress ambient cloud to form stars. I will use Chandra, XMM-Newton, FUSE, HST, Spitzer, ATCA, and other ground-based observations to illustrate the interplay among massive stars, interstellar medium, and star formation.

Keywords

ISM: bubblesISM: evolutionISM: generalgalaxies: ISMMagellanic Clouds
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S256: The Magellanic System: Stars, Gas, and Galaxies , July 2008 , pp. 166 - 177
Copyright
Copyright © International Astronomical Union 2009

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