The Multiple-Phase Structure of the Interstellar Medium in the Large Magellanic Cloud

Details The Multiple-Phase Structure of the Interstellar Medium in the Large Magellanic Cloud The Multiple-Phase Structure of the Interstellar Medium in the Large Magellanic Cloud

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108..393s&link_type=abstract

Structure and Evolution of the Magellanic Clouds, Proceedings of IAU Symposium No. 108, held 5-8 September 1983 in Tübingen, Wes

Physics

Scientific paper

Physical properties of the ISM near SNRs in the LMC can be deduced from
high-resolution, two-dimensional spectra. The ISM around the N49 and
N63A SNRs apparently has as many as three different phases of varying
density, clumpiness, and spatial distribution.

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