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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.

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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