You-Hua Chu, PASA, 15 (1), 136
The html and gzipped postscript versions of this paper are in preprint form.
To access the final published version, download the pdf file.
Next Section: Introduction
Multi-Wavelength View of the Interstellar Medium in the Large Magellanic Cloud
You-Hua Chu
Astronomy Dept., Univ. of Illinois, 1002 W. Green Street, Urbana, IL 61801, USA
chu@astro.uiuc.edu
Abstract:
The Large Magellanic Cloud (LMC) has been surveyed in optical emission lines, X-rays, radio continuum, HI, and CO lines. These surveys provide unprecedentedly clear views of the interstellar medium (ISM) in the LMC, 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 Clouds - galaxies: ISM - ISM: general - ISM: structure - ISM: bubbles - supernova remnants
HTML Section | Download Full Paper |
---|---|
б© Copyright Astronomical Society of Australia 1997