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The Physics of 106 K Gas in LMC Supergiant Shells

Published online by Cambridge University Press:  25 May 2016

D. J. Bomans  and
K. Dennerl
D. J. Bomans
Affiliation:
Astronomisches Institut, Ruhr-Universität Bochum, Germany
K. Dennerl
Affiliation:
MPI für extraterrestrische Physik, Garching, Germany

Abstract

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We present first results of our study of the interplay between the 106 K, 104 K, 102 K gas phases in the supergiant shell LMC 4.

Type
Part 2. Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 158 - 159
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Bomans, D.J., Dennerl, K, & Kürster, M. 1993, A&A, 283, L21 Google Scholar
Bomans, D.J., de Boer, K.S., Koornneef, J., & Grebel, E.K. 1996, A&A, 313. 101 Google Scholar
Braunsfurth, E., & Feitzinger, J.V. 1983, A&A, 123, 113 Google Scholar
Chu, Y.-H., & Mac Low, M.-M. 1990, ApJ, 365, 510 Google Scholar
Domgoergen, H., Bomans, D.J., & de Boer, K.S. 1995, A&A, 296, 523 Google Scholar
Mac Low, M.-M., McCray, R., & Norman, M.L. 1989, ApJ, 337, 141 CrossRefGoogle Scholar
Meaburn, J. 1980, MNRAS, 192, 365 Google Scholar
Weaver, R., McCray, R., Castor, J., Shapiro, P., & Moore, R. 1978, ApJ, 218. 377 Google Scholar
Wheelock, et al. 1991, IRAS Sky Survey Atlas Explanatory Supplement Google Scholar