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The Multiple-Phase Structure of the Interstellar Medium in the LMC

Published online by Cambridge University Press:  04 August 2017

P. Shull Jr.
P. Shull Jr.*
Affiliation:
Max-Planck-Institut für Astronomie

Extract

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

Information

Type
Interstellar Matter
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 393 - 394
Copyright
Copyright © Reidel 1984 

References

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