Multi-wavelength view of the interstellar medium in the Large Magellanic Cloud

Details Multi-wavelength view of the interstellar medium in the Large Magellanic Cloud Multi-wavelength view of the interstellar medium in the Large Magellanic Cloud

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998pasa...15..136c&link_type=abstract

Publications Astronomical Society of Australia, vol. 15, no. 1, p. 136-40

Astronomy and Astrophysics

Astronomy

Magellanic Clouds, Interstellar Medium, Supernova Remnants

Scientific paper

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.

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